List of stars in Carina

This is the list of notable stars in the constellation Carina, sorted by decreasing brightness.

This constellation's Bayer designations (Greek-letter star names) were given while it was still considered part of the constellation of Argo Navis. After Argo Navis was broken up into Carina, Vela, and Puppis, these Greek-letter designations were kept, so that Carina does not have a full complement of Greek-letter designations. For example, since Argo Navis's gamma star went to Vela, there is no Gamma Carinae.

Name

B

Var

HD

HIP

RA

Dec

Dist. (ly)

Notes

α

45348

30438

06^h 23^m 57.09^s

−52° 41′ 44.6″

−0.72

−5.53

313

A9 II^[1]^[2]

Suhel;^[3] 2nd brightest star

β Car

β

80007

45238

09^h 13^m 12.24^s

−69° 43′ 02.9″

1.67

−0.99

111

A1 III^[4]

Miaplacidus

ε Car

ε

71129

41037

08^h 22^m 30.86^s

−59° 30′ 34.3″

1.86

−4.58

632

K3III+B2V

Avior; suspected eclipsing binary, V_max = 1.82^m, V_min = 1.94^m

ι Car

ι

80404

45556

09^h 17^m 05.43^s

−59° 16′ 30.9″

2.23

−4.43

692

A8Ib

Aspidiske, Turais, Scutulum; suspected variable, V_max = 2.23^m, V_min = 2.28^m

θ Car

θ

93030

52419

10^h 42^m 57.43^s

−64° 23′ 40.1″

2.74

−2.91

439

B0Vp

in IC 2602

υ Car

υ

85123

48002

09^h 47^m 06.14^s

−65° 04′ 19.3″

2.92

−5.56

1622

A9

binary star

ω Car

ω

89080

50099

10^h 13^m 44.28^s

−70° 02′ 16.5″

3.29

−1.99

370

B8III

p Car

p

PP

91465

51576

10^h 32^m 01.48^s

−61° 41′ 07.3″

3.30

−2.62

497

B4Vne

γ Cas variable, V_max = 3.22^m, V_min = 3.55^m

V337 Car

q

V337

89388

50371

10^h 17^m 05.01^s

−61° 19′ 56.4″

3.39

−3.38

736

K3II

irregular variable, V_max = 3.36^m, V_min = 3.44^m

a Car

a

V357

79351

45080

09^h 10^m 58.11^s

−58° 58′ 00.9″

3.43

−2.11

418

B2IV

eclipsing binary, V_max = 3.41^m, V_min = 3.44^m

χ Car

χ

65575

38827

07^h 56^m 46.74^s

−52° 58′ 56.6″

3.46

−1.91

387

B3IVp

β Cep variable, ΔV = 0.015^m, P = 0.10 d

l Car

l

84810

47854

09^h 45^m 14.83^s

−62° 30′ 28.5″

3.69

−4.64

1509

G5Iab/Ib

classical Cepheid, V_max = 3.28^m, V_min = 4.18^m, P = 35.54 d

HD 94510

u

94510

53253

10^h 53^m 29.57^s

−58° 51′ 11.8″

3.78

1.42

97

K0III-IV...

suspected variable, V_max = 3.75^m, V_min = 3.80^m

HD 90853

s

90853

51232

10^h 27^m 52.75^s

−58° 44′ 21.9″

3.81

−3.71

1042

F2II

suspected variable

HD 76728

c

76728

43783

08^h 55^m 02.86^s

−60° 38′ 41.0″

3.84

−1.06

312

B8III

double star

V382 Car

x

V382

96918

54463

11^h 08^m 35.40^s

−58° 58′ 30.2″

3.93

−7.37

5927

G0Ia0

hypergiant; slow irregular variable, V_max = 3.77^m, V_min = 4.05^m

HD 79447

i

79447

45101

09^h 11^m 16.77^s

−62° 19′ 01.3″

3.96

−1.97

499

B3IV

variable star, ΔV = 0.008^m, P = 22.26 d

HD 90589

I

90589

50954

10^h 24^m 23.74^s

−74° 01′ 53.6″

3.99

2.94

53

F2IV

suspected variable, V_max = 3.96^m, V_min = 4.00^m

HD 83183

h

83183

46974

09^h 34^m 26.66^s

−59° 13′ 47.2″

4.08

−4.83

1976

B5II

V343 Car

d

V343

74375

42568

08^h 40^m 37.04^s

−59° 45′ 39.7″

4.31

−3.87

1411

B1.5III

β Cep variable

HD 80230

g

80230

45496

09^h 16^m 12.10^s

−57° 32′ 29.2″

4.34

−1.74

536

M1III

suspected variable, V_max = 4.31^m, V_min = 4.35^m

HD 47306

N

47306

31407

06^h 34^m 58.59^s

−52° 58′ 32.3″

4.35

−4.31

1762

B9III

HR 2554

A

V415

50337

32761

06^h 49^m 51.32^s

−53° 37′ 21.0″

4.39

−1.74

553

G6II

Algol variable, ΔV = 0.06^m

HD 91942

r

91942

51849

10^h 35^m 35.31^s

−57° 33′ 27.5″

4.45

−3.68

1376

K3/K4II

suspected variable

η Car

η

93308

10^h 45^m 03.60^s

−59° 41′ 03.0″

4.47

7500

LBV

Foramen, Tseen She; in Trumpler 16; binary star; luminous blue variable, V_max = −0.8^m, V_min = 7.9^m; surrounded by the Homunculus Nebula; one of the most luminous and most massive stars known.

HR 3643

G

78791

44599

09^h 05^m 08.83^s

−72° 36′ 09.7″

4.47

−1.25

454

F6II-III

V344 Car

f

V344

75311

43105

08^h 46^m 42.56^s

−56° 46′ 11.3″

4.50

−1.62

546

B3Vne

γ Cas variable, V_max = 4.40^m, V_min = 4.51^m

HD 83944

m

83944

47391

09^h 39^m 21.04^s

−61° 19′ 41.2″

4.51

0.33

224

B9V

suspected variable

V520 Car

w

V520

93070

52468

10^h 43^m 32.31^s

−60° 33′ 59.9″

4.58

−2.99

1065

K3Ib

irregular variable, V_max = 4.50^m, V_min = 4.59^m

V533 Car

y

V533

97534

54751

11^h 12^m 36.02^s

−60° 19′ 03.5″

4.59

−8.34

12538

A6Ia

α Cyg variable

HD 96566

z¹

96566

54301

11^h 06^m 32.47^s

−62° 25′ 26.9″

4.62

−0.65

370

G8III

V399 Car

P

V399

90772

51192

10^h 27^m 24.48^s

−57° 38′ 19.7″

4.65

A6Ia

semiregular variable, V_max = 4.63^m, V_min = 4.72^m, P = 88.3 d

V345 Car

E

V345

78764

44626

09^h 05^m 38.38^s

−70° 32′ 18.7″

4.67

−2.94

1079

B2IVe

γ Cas variable, V_max = 4.67^m, V_min = 4.78^m, P = 137.7 d

HD 92397

t²

92397

52102

10^h 38^m 45.01^s

−59° 10′ 58.8″

4.69

−4.08

1852

K4/K5III:

suspected variable

HD 91375

K

91375

51438

10^h 30^m 20.08^s

−71° 59′ 33.8″

4.72

0.22

259

A2III

HR 3220

B

68456

39903

08^h 09^m 00.86^s

−61° 18′ 06.1″

4.74

3.09

70

F5V

V518 Car

V518

92938

52370

10^h 42^m 14.14^s

−64° 27′ 59.2″

4.76

−0.97

456

B3V

in IC 2602; γ Cas variable

HD 81101

k

81101

45856

09^h 20^m 56.83^s

−62° 24′ 16.7″

4.79

0.62

223

G6III

HD 93194

93194

52502

10^h 44^m 06.94^s

−63° 57′ 40.0″

4.80

−1.06

484

B5Vn

in IC 2602; suspected irregular variable, V_max = 4.79^m, V_min = 4.84^m

HD 66591

D

66591

39138

08^h 00^m 19.97^s

−63° 34′ 03.0″

4.81

−1.29

542

B3V

suspected variable

HD 73389

e²

73389

42134

08^h 35^m 19.65^s

−58° 00′ 33.5″

4.84

0.60

229

K0III

HD 93607

93607

52736

10^h 46^m 51.24^s

−64° 23′ 00.6″

4.87

−0.83

449

B3IV

in IC 2602; suspected variable

HD 61248

Q

61248

36942

07^h 35^m 39.70^s

−52° 32′ 01.7″

4.93

−0.48

394

K3III

suspected variable

V376 Car

b¹

V376

77002

43937

08^h 56^m 58.43^s

−59° 13′ 45.7″

4.93

−1.47

621

B2IV-V

β Cep variable, V_max = 4.91^m, V_min = 4.96^m, P = 0.021 d

HD 91496

91496

51495

10^h 31^m 02.07^s

−73° 13′ 17.4″

4.94

−2.42

964

K4/K5III

suspected variable, V_max = 4.87^m, V_min = 4.97^m

HD 90264

L

90264

50847

10^h 22^m 58.18^s

−66° 54′ 05.5″

4.97

−0.63

430

B8V

HD 92063

t¹

92063

51912

10^h 36^m 20.56^s

−59° 33′ 51.5″

5.08

0.50

269

K1III

HD 59219

59219

36114

07^h 26^m 21.86^s

−51° 01′ 06.6″

5.09

−1.09

562

K0III

HD 96919

z²

V371

96919

54461

11^h 08^m 34.01^s

−61° 56′ 49.8″

5.12

−6.03

5525

B9Ia

α Cyg variable, V_max = 5.12^m, V_min = 5.19^m

HD 53047

53047

33779

07^h 00^m 51.51^s

−51° 24′ 09.5″

5.14

−1.25

617

M1III

semiregular variable

V386 Car

V386

54118

34105

07^h 04^m 18.32^s

−56° 44′ 59.0″

5.14

0.45

282

A0p:

α² CVn variable, ΔV = 0.026^m, P = 3.28 d

HD 88981

M

88981

50083

10^h 13^m 30.68^s

−66° 22′ 22.2″

5.15

0.31

304

Am

HD 69863

C

69863

40429

08^h 15^m 15.95^s

−62° 54′ 56.2″

5.16

0.81

242

A+...

binary star

HD 77370

b²

77370

44143

08^h 59^m 24.38^s

−59° 05′ 03.8″

5.17

3.08

85

F3V

HR 3153

V460

66342

39070

07^h 59^m 37.55^s

−60° 35′ 13.5″

5.19

−2.34

1045

M0II

in NGC 2516; semiregular variable, V_max = 5.15^m, V_min = 5.3^m

HD 97583

97583

54767

11^h 12^m 45.27^s

−64° 10′ 11.2″

5.22

0.30

314

B9V

double star

HD 93549

93549

52701

10^h 46^m 29.61^s

−64° 15′ 47.7″

5.23

−0.37

429

B7IV

in IC 2602

HD 88323

88323

49698

10^h 08^m 42.84^s

−65° 48′ 55.9″

5.26

0.16

341

K0III

optical double

V524 Car

V524

94367

53154

10^h 52^m 30.85^s

−57° 14′ 25.5″

5.26

−6.08

6037

B9Ia

α Cyg variable

HD 73390

e¹

73390

42129

08^h 35^m 15.58^s

−58° 13′ 29.1″

5.27

−2.08

962

B3V+...

HD 91056

91056

51313

10^h 28^m 52.60^s

−64° 10′ 20.2″

5.27

−4.64

3135

K3Ib

slow irregular variable

HD 80951

80951

45581

09^h 17^m 25.21^s

−74° 53′ 39.8″

5.28

−1.44

721

A1V

HD 84121

84121

47479

09^h 40^m 42.60^s

−57° 59′ 00.9″

5.30

1.16

220

A3IV

HD 93540

93540

52678

10^h 46^m 16.58^s

−64° 30′ 52.5″

5.33

−0.45

466

B7:V

in IC 2602; suspected variable

HD 92964

V519

92964

52405

10^h 42^m 40.57^s

−59° 12′ 56.8″

5.36

−6.23

6792

B2.5Ia

α Cyg variable, V_max = 5.32^m, V_min = 5.43^m, P = 14.68 d

HD 57917

57917

35589

07^h 20^m 38.81^s

−52° 05′ 09.3″

5.38

−0.52

493

B9V

HD 80671

80671

45571

09^h 17^m 17.40^s

−68° 41′ 22.5″

5.38

2.75

109

F4V

HD 49689

49689

32494

06^h 46^m 52.69^s

−51° 15′ 55.6″

5.39

−1.83

906

K1II/IIIp+G:

suspected variable

HD 73887

73887

42286

08^h 37^m 18.85^s

−62° 51′ 12.3″

5.45

0.39

335

K0III

HD 82350

82350

46358

09^h 27^m 06.50^s

−71° 36′ 07.5″

5.46

1.51

201

K2III

HD 83095

H

83095

46741

09^h 31^m 36.32^s

−73° 04′ 51.3″

5.46

−1.47

791

K4III

HD 92207

V370

92207

52004

10^h 37^m 27.08^s

−58° 44′ 00.0″

5.47

−6.52

8150

A0Ia

α Cyg variable, V_max = 5.45^m, V_min = 5.52^m, P = 1.33 d

V450 Car

V450

53921

34000

07^h 03^m 15.11^s

−59° 10′ 41.3″

5.50

−0.35

482

B9IV

53 Per variable, ΔV = 0.02^m

HD 92664

V364

92664

52221

10^h 40^m 11.46^s

−65° 06′ 00.9″

5.51

−0.26

466

B9p Si

α² CVn variable, V_max = 5.48^m, V_min = 5.52^m, P = 1.67 d

HD 67364

67364

39566

08^h 05^m 03.71^s

−53° 06′ 28.5″

5.52

0.11

393

K3/K4III

HD 79698

79698

45219

09^h 12^m 55.62^s

−59° 24′ 50.3″

5.54

−0.28

475

G6II

HD 85656

85656

48310

09^h 50^m 55.60^s

−62° 44′ 42.5″

5.56

−1.78

959

K1IIICN...

HD 64067

64067

38152

07^h 49^m 06.72^s

−56° 24′ 37.4″

5.57

−1.72

934

G5II

HD 46569

46569

31079

06^h 31^m 18.22^s

−51° 49′ 34.3″

5.58

2.73

121

F8V

HD 96706

96706

54327

11^h 06^m 49.93^s

−70° 52′ 40.6″

5.58

−2.12

1128

B2V

variable star, ΔV = 0.004^m, P = 1.74 d

HD 65907

65907

38908

07^h 57^m 46.30^s

−60° 18′ 12.1″

5.59

4.54

53

G2V...

HD 76113

76113

43499

08^h 51^m 36.53^s

−57° 38′ 01.0″

5.59

−1.12

716

B8III

V448 Car

O

V448

49877

32531

06^h 47^m 18.71^s

−55° 32′ 24.2″

5.60

−0.72

598

K5III

semiregular variable

HD 65273

65273

38656

07^h 54^m 53.39^s

−57° 18′ 10.4″

5.62

0.51

343

K3/K4III

HD 68434

68434

39957

08^h 09^m 33.63^s

−56° 05′ 07.7″

5.66

0.33

380

A3m...

HD 89715

89715

50520

10^h 19^m 05.12^s

−64° 40′ 34.6″

5.66

0.90

292

A1V

V372 Car

V372

64722

38438

07^h 52^m 29.75^s

−54° 22′ 01.9″

5.69

−2.56

1462

B1.5IV

β Cep variable, ΔV = 0.027^m, P = 0.12 d

HD 88661

QY

88661

49934

10^h 11^m 46.47^s

−58° 03′ 38.0″

5.70

−2.29

1294

B2IVnpe

γ Cas variable, V_max = 5.63^m, V_min = 5.83^m

S Car

S

88366

49751

10^h 09^m 22.01^s

−61° 32′ 57.1″

5.71

1780

K5-M6e

Mira variable, V_max = 4.5^m, V_min = 9.9^m, P = 149.49 d

HD 97670

97670

54829

11^h 13^m 30.79^s

−59° 37′ 09.5″

5.73

−3.00

1821

B1.5V

suspected variable

HD 65662

65662

38783

07^h 56^m 18.65^s

−60° 31′ 35.3″

5.74

−2.17

1244

K4II

in NGC 2516

HD 93163

93163

52487

10^h 43^m 51.21^s

−64° 14′ 56.6″

5.75

−1.71

1009

B3:V

suspected eclipsing binary, ΔV = 0.03^m

HD 66194

V374

66194

38994

07^h 58^m 50.56^s

−60° 49′ 28.2″

5.77

−1.72

1028

B2IVnpe

in NGC 2516; γ Cas variable, V_max = 5.72^m, V_min = 5.84^m

HD 81830

81830

46225

09^h 25^m 27.38^s

−61° 57′ 02.2″

5.77

1.47

236

A4V+...

HD 64185

64185

38160

07^h 49^m 12.95^s

−60° 17′ 02.5″

5.78

3.06

114

F1V

spectroscopic binary

HD 76538

76538

43669

08^h 53^m 48.67^s

−60° 21′ 14.2″

5.78

−2.35

1376

B5III

HD 85655

85655

48339

09^h 51^m 12.03^s

−59° 25′ 32.4″

5.79

−1.01

746

K2IIICNp...

HD 77615

77615

44256

09^h 00^m 45.75^s

−60° 57′ 49.8″

5.80

−2.13

1259

G8II

HD 84152

84152

47498

09^h 41^m 02.10^s

−57° 15′ 34.0″

5.80

0.57

362

K0/K1III

HD 88473

88473

49764

10^h 09^m 30.20^s

−68° 40′ 58.2″

5.80

−0.46

583

A0IV

HD 49517

49517

32402

06^h 45^m 53.72^s

−52° 24′ 35.0″

5.81

−2.32

1376

K3III

HD 93943

93943

52922

10^h 49^m 24.46^s

−59° 19′ 25.6″

5.85

−1.24

853

B9.5IV/V

HD 80950

80950

45585

09^h 17^m 27.63^s

−74° 44′ 04.8″

5.86

1.32

264

A0V

HD 60060

60060

36444

07^h 29^m 59.74^s

−52° 39′ 04.6″

5.87

0.84

330

K0III

HD 66441

66441

39184

08^h 00^m 49.96^s

−54° 09′ 04.7″

5.87

−0.79

700

B5Vn

suspected variable

V482 Car

V482

82536

46620

09^h 30^m 23.45^s

−58° 21′ 42.9″

5.88

−1.68

1058

M2III

semiregular variable

V514 Car

V514

92287

52043

10^h 38^m 02.66^s

−57° 15′ 22.7″

5.89

−2.08

1278

B3IV

rotating ellipsoidal variable, V_max = 5.88^m, V_min = 5.92^m, P = 2.90 d

HD 82406

82406

46460

09^h 28^m 30.60^s

−66° 42′ 07.2″

5.90

1.33

268

A0V

HD 82347

82347

46482

09^h 28^m 47.19^s

−62° 16′ 23.5″

5.91

0.06

482

K1III

HD 87283

87283

49164

10^h 02^m 00.11^s

−60° 25′ 15.2″

5.93

−4.03

3196

A9IV

possibly in NGC 3114

HD 90454

90454

50993

10^h 24^m 59.50^s

−58° 34′ 34.7″

5.93

1.13

297

F2III

T Car

T

94776

53394

10^h 55^m 17.26^s

−60° 31′ 01.9″

5.93

1.07

306

K0III

not variable

HD 60228

60228

36496

07^h 30^m 30.91^s

−54° 23′ 58.0″

5.95

0.33

433

M1III

HD 94683

94683

53334

10^h 54^m 29.60^s

−61° 49′ 35.8″

5.95

−2.59

1663

K4III

suspected variable

HD 54732

54732

34349

07^h 07^m 13.30^s

−51° 58′ 06.2″

5.96

−0.23

564

K0III

HD 56705

56705

35084

07^h 15^m 21.27^s

−52° 29′ 58.3″

5.96

0.58

389

K0V

HD 70839

70839

40932

08^h 21^m 12.10^s

−57° 58′ 23.6″

5.96

−3.36

2380

B1.5III

HD 92436

92436

52127

10^h 38^m 59.70^s

−58° 49′ 00.8″

5.96

−0.53

648

M1III

HD 91533

91533

51623

10^h 32^m 47.82^s

−58° 40′ 00.3″

5.98

−6.71

11241

A2Iab

suspected variable

V522 Car

V522

93737

52827

10^h 48^m 05.42^s

−59° 55′ 09.0″

5.98

A0Ia

α Cyg variable

HD 81613

81613

46101

09^h 24^m 05.50^s

−61° 38′ 55.6″

5.99

0.92

337

K0III

HD 94650

94650

53272

10^h 53^m 42.13^s

−70° 43′ 13.2″

5.99

−0.89

776

B6V

HD 98560

98560

55280

11^h 19^m 16.84^s

−64° 34′ 57.4″

5.99

3.12

122

F6IV

HD 90874

90874

51194

10^h 27^m 25.40^s

−65° 42′ 17.0″

6.00

1.76

229

A2V

HD 53349

53349

33800

07^h 01^m 05.18^s

−58° 56′ 25.1″

6.01

2.36

175

F0V

suspected variable

HD 76346

76346

43620

08^h 53^m 03.80^s

−56° 38′ 58.5″

6.02

1.23

296

A0V

has a planet (b)

HD 80094

80094

45418

09^h 15^m 17.66^s

−58° 23′ 18.2″

6.02

0.00

522

B7IV

variable star, ΔV = 0.008^m, P = 1.56 d

HD 56239

56239

34780

07^h 12^m 01.98^s

−63° 11′ 24.2″

6.03

−0.29

598

A0IV/V

HD 57852

57852

35564

07^h 20^m 21.46^s

−52° 18′ 42.8″

6.05

113

F5V

component of the HIP 35564 system; suspected variable

HD 82068

82068

46328

09^h 26^m 44.18^s

−64° 55′ 47.5″

6.05

1.88

223

A3Vn

V390 Car

V390

61966

37248

07^h 39^m 00.34^s

−53° 16′ 24.2″

6.06

−0.05

544

B9IV-Vp...

α² CVn variable, ΔV = 0.004^m

V535 Car

V535

98292

55140

11^h 17^m 19.02^s

−67° 49′ 24.6″

6.06

−2.52

1698

M2III

slow irregular variable

HD 88825

88825

50044

10^h 13^m 01.16^s

−59° 55′ 05.1″

6.07

−2.84

1976

B4Ve

HD 96544

96544

54294

11^h 06^m 29.30^s

−58° 40′ 30.1″

6.07

−1.81

1226

K2II/III

HD 92682

92682

52150

10^h 39^m 15.94^s

−74° 29′ 36.2″

6.08

−1.57

1105

K3II

variable star, ΔV = 0.005^m, P = 0.084 d

HD 63382

63382

37854

07^h 45^m 35.52^s

−56° 43′ 21.3″

6.10

−1.20

942

F0II

R Car

R

82901

46806

09^h 32^m 14.60^s

−62° 47′ 20.0″

6.10

416

M6.5 IIIpev

Mira variable, V_max = 3.9^m, V_min = 10.5^m, P = 308.71 d

HD 91619

V369

91619

51676

10^h 33^m 25.40^s

−58° 11′ 24.6″

6.11

−6.99

13583

B7Ia

α Cyg variable, ΔV = 0.1^m, P = 1.12 d

U Car

U

95109

53589

10^h 57^m 48.19^s

−59° 43′ 55.9″

6.11

G3Ia

classical Cepheid, V_max = 5.74^m, V_min = 6.96^m, P = 38.83 d

HD 70982

70982

40926

08^h 21^m 07.65^s

−64° 06′ 21.4″

6.11

0.34

464

G6/G8III

V461 Car

V461

66546

39225

08^h 01^m 23.05^s

−54° 30′ 56.0″

6.12

−1.92

1320

B2IV-V

Algol variable

HD 65908

65908

38863

07^h 57^m 12.76^s

−63° 17′ 48.8″

6.14

0.37

464

B8V

V478 Car

V478

80710

45615

09^h 17^m 51.67^s

−67° 03′ 03.2″

6.14

−1.96

1358

K2III

semiregular variable

HD 87543

87543

49281

10^h 03^m 34.14^s

−61° 53′ 02.6″

6.14

−2.49

1734

B4:Vne

HD 95208

95208

53546

10^h 57^m 15.81^s

−75° 05′ 59.2″

6.16

−3.12

2345

K1II

HD 95324

95324

53701

10^h 59^m 14.05^s

−61° 19′ 14.7″

6.16

0.93

363

B8IV

HD 96088

96088

54082

11^h 04^m 00.25^s

−57° 57′ 19.2″

6.16

−3.63

2964

B3III

HD 47001

47001

31265

06^h 33^m 26.31^s

−52° 19′ 45.5″

6.18

−0.17

607

G8III

V492 Car

V492

86659

48782

09^h 56^m 59.84^s

−69° 06′ 06.6″

6.18

−1.43

1087

B3V

53 Per variable

HD 87436

87436

49233

10^h 02^m 59.95^s

−60° 10′ 43.3″

6.18

−3.80

3228

A6II/III

suspected variable

HD 90630

90630

50976

10^h 24^m 44.56^s

−73° 58′ 18.3″

6.18

0.53

441

A2/A3V

suspected variable

V655 Car

V655

91272

51425

10^h 30^m 08.81^s

−66° 59′ 04.8″

6.19

−1.70

1235

B4IV

Algol variable, V_max = 6.19^m, V_min = 6.36^m, P = 16.93 d

HD 62897

62897

37599

07^h 42^m 53.36^s

−58° 13′ 48.5″

6.20

−0.23

629

K0III

HD 75086

75086

42936

08^h 45^m 05.55^s

−58° 43′ 27.6″

6.20

−1.23

997

B7III

HD 87238

87238

49160

10^h 01^m 58.09^s

−57° 20′ 59.4″

6.20

−0.62

753

K1II

HD 84850

84850

47913

09^h 45^m 55.82^s

−58° 47′ 38.4″

6.22

1.68

264

F5IV

HD 89263

89263

50287

10^h 16^m 03.26^s

−59° 54′ 12.4″

6.22

1.63

270

A5V

V532 Car

V532

97451

54708

11^h 12^m 03.60^s

−58° 25′ 24.1″

6.24

−0.53

736

M4III

semiregular variable

HD 91767

91767

51732

10^h 34^m 12.72^s

−60° 59′ 15.5″

6.25

−0.78

830

K2/K3III

suspected variable

HD 65750

V341

65750

38834

07^h 56^m 50.70^s

−59° 07′ 35.0″

6.25

967

M0III

semiregular variable, V_max = 6.2^m, V_min = 7.1^m

HD 93344

93344

52520

10^h 44^m 20.10^s

−70° 51′ 35.0″

6.25

1.12

346

A5IV/V

HD 52603

52603

33588

06^h 58^m 39.81^s

−55° 43′ 44.1″

6.26

1.59

280

K2III

HD 74622

74622

42717

08^h 42^m 20.90^s

−55° 46′ 28.8″

6.26

1.23

331

K2III

υ Car B

υ

85124

09^h 47^m 06.70^s

−65° 04′ 21.0″

6.26

1623

A8 Ib

component of the υ Car system

HD 93372

93372

52535

10^h 44^m 27.25^s

−72° 26′ 37.1″

6.26

3.74

104

F6V

HD 93502

93502

52679

10^h 46^m 17.12^s

−60° 36′ 10.4″

6.26

1.01

365

A0IV

HD 94491

94491

53231

10^h 53^m 21.18^s

−58° 53′ 36.5″

6.26

−2.16

1575

B5V

HD 82858

82858

46737

09^h 31^m 33.05^s

−66° 43′ 08.6″

6.27

−0.40

703

K1III

HD 66607

66607

39238

08^h 01^m 31.58^s

−55° 27′ 16.8″

6.28

−0.28

668

B4V

V375 Car

V375

67536

39530

08^h 04^m 42.94^s

−62° 50′ 10.9″

6.29

1249

B2.5Vn

β Cep variable, ΔV = 0.04^m, P = 1.02 d

HD 61031

61031

36856

07^h 34^m 39.58^s

−51° 28′ 28.3″

6.29

−1.76

1331

A1III/IV

HD 93662

93662

52797

10^h 47^m 38.41^s

−57° 28′ 02.7″

6.29

−3.35

2763

M1II

suspected variable, V_max = 6.28^m, V_min = 6.41^m

HD 94275

94275

53100

10^h 51^m 46.93^s

−57° 16′ 20.3″

6.29

−0.05

604

A6III

HD 63926

63926

38087

07^h 48^m 19.51^s

−56° 28′ 15.9″

6.30

−2.91

2264

K0III+...

HD 66341

66341

39073

07^h 59^m 40.09^s

−60° 12′ 26.6″

6.30

−1.81

1364

B8III

in NGC 2516

HD 81502

81502

46049

09^h 23^m 27.33^s

−60° 18′ 08.4″

6.30

−2.91

2264

K1/K2II/III

HD 86606

86606

48715

09^h 56^m 09.76^s

−71° 23′ 21.5″

6.30

−2.69

2050

B1Ib

HD 68423

68423

39843

08^h 08^m 24.65^s

−63° 48′ 03.0″

6.32

−0.58

782

B6V

suspected variable

HD 80126

80126

45437

09^h 15^m 34.73^s

−57° 34′ 39.9″

6.32

−1.32

1098

G8II

QZ Car

QZ

93206

52526

10^h 44^m 22.92^s

−59° 59′ 36.0″

6.32

−3.23

2650

B0Ib:

in Collinder 228; β Lyr variable, V_max = 6.16^m, V_min = 6.49^m, P = 6.00 d

HD 82458

82458

46407

09^h 27^m 49.19^s

−71° 46′ 52.3″

6.33

2.57

184

F3/F5V

V486 Car

V486

84416

47591

09^h 42^m 12.99^s

−66° 54′ 53.4″

6.33

0.04

592

A0V

β Lyr variable

HD 92536

92536

52160

10^h 39^m 22.85^s

−64° 06′ 42.5″

6.33

0.49

479

B8V

in IC 2602

HD 74341

74341

42579

08^h 40^m 43.55^s

−57° 32′ 43.9″

6.34

2.13

227

A3V

HD 90074

90074

50785

10^h 22^m 10.48^s

−58° 15′ 56.3″

6.34

1.23

343

G6III

HD 90289

90289

50916

10^h 23^m 50.66^s

−57° 57′ 14.1″

6.34

−0.59

793

K5Ib-II

suspected variable, V_max = 6.33^m, V_min = 6.35^m

HD 93649

93649

52730

10^h 46^m 48.09^s

−69° 12′ 35.3″

6.34

−2.04

1545

A2IV

HD 97472

97472

54673

11^h 11^m 29.57^s

−71° 26′ 10.3″

6.34

0.08

583

K2/K3III

HD 74148

74148

42440

08^h 39^m 13.24^s

−60° 19′ 02.4″

6.35

0.71

437

A0V

HD 89805

89805

50562

10^h 19^m 42.04^s

−65° 08′ 14.1″

6.35

−2.59

2000

K2II

WR 22

V429

92740

52308

10^h 41^m 17.52^s

−59° 40′ 36.9″

6.35

−4.72

5344

WN7 + A(SB1)

Wolf–Rayet star and Algol variable, V_max = 6.33^m, V_min = 6.52^m, P = 80.34 d; one of the most luminous stars known

HD 93739

93739

52785

10^h 47^m 30.62^s

−69° 26′ 15.8″

6.35

−1.57

1249

B2IV

HD 65189

65189

38667

07^h 55^m 00.44^s

−52° 35′ 00.1″

6.36

−1.08

1003

B8III

HD 72322

72322

41653

08^h 29^m 36.40^s

−55° 11′ 27.3″

6.36

−0.36

721

G0V

V473 Car

V473

76640

43763

08^h 54^m 54.05^s

−58° 14′ 22.9″

6.36

−0.77

869

B5V

53 Per variable

HD 79699

79699

45214

09^h 12^m 50.63^s

−60° 55′ 00.5″

6.36

0.21

553

B9V

HD 78632

78632

44665

09^h 06^m 07.61^s

−64° 29′ 59.7″

6.37

0.08

590

K3III

HD 61394

61394

36977

07^h 36^m 01.62^s

−55° 53′ 15.8″

6.39

0.06

601

K1/K2IIICN.

HD 96568

96568

54289

11^h 06^m 24.32^s

−64° 50′ 23.8″

6.39

0.58

473

A3V

HD 44267

44267

29913

06^h 17^m 51.74^s

−52° 43′ 58.9″

6.40

−0.70

858

K2/K3III

variable star, ΔV = 0.008^m, P = 1.32 d

HD 62758

62758

37530

07^h 42^m 10.22^s

−58° 37′ 51.4″

6.40

−1.18

1069

B2.5V

V368 Car

V368

88647

49926

10^h 11^m 35.49^s

−58° 49′ 40.2″

6.40

801

M3III

semiregular variable, V_max = 6.1^m, V_min = 6.4^m

HD 51210

51210

33012

06^h 52^m 45.44^s

−59° 20′ 28.6″

6.41

0.62

470

A3m...

HD 87438

87438

49223

10^h 02^m 49.42^s

−62° 09′ 24.0″

6.41

−3.23

2763

K3Ib

irregular variable, V_max = 6.38^m, V_min = 6.43^m

HD 91270

91270

51461

10^h 30^m 39.24^s

−61° 21′ 23.4″

6.41

−0.57

811

M2III

suspected variable

HD 84046

84046

47422

09^h 39^m 45.15^s

−62° 56′ 34.7″

6.42

0.01

623

B8/B9III/IVw...

suspected variable, V_max = 6.42^m, V_min = 6.8^m

HD 88907

88907

50067

10^h 13^m 21.20^s

−61° 39′ 31.8″

6.42

−1.06

1022

B2V

V507 Car

V507

90966

51265

10^h 28^m 18.28^s

−63° 09′ 52.5″

6.42

−2.56

2037

B2/B3III:ne

Be star

HD 91094

91094

51327

10^h 29^m 03.67^s

−65° 10′ 34.8″

6.42

0.00

627

M1III

semiregular variable

HD 98025

98025

55003

11^h 15^m 42.76^s

−57° 21′ 21.1″

6.42

0.16

583

A3V

HD 78293

78293

44565

09^h 04^m 48.00^s

−57° 51′ 09.5″

6.43

−1.21

1101

A8III

HD 93359

93359

52537

10^h 44^m 32.42^s

−70° 51′ 18.9″

6.43

1.25

354

A6IV

HD 65867

65867

38963

07^h 58^m 21.47^s

−51° 26′ 54.9″

6.44

0.43

518

A8/A9IV

suspected eclipsing binary

V469 Car

V469

72303

41644

08^h 29^m 29.82^s

−54° 12′ 42.5″

6.44

−0.28

720

Ap Si

α² CVn variable

HD 49705

49705

32477

06^h 46^m 41.70^s

−54° 41′ 42.2″

6.45

0.93

414

G6III

HD 81896

81896

46143

09^h 24^m 37.16^s

−70° 04′ 32.8″

6.45

0.06

617

K1III

V495 Car

V495

88158

49642

10^h 07^m 56.64^s

−62° 13′ 17.2″

6.45

−0.55

817

Ap Si

α² CVn variable

WR 24

93131

52488

10^h 43^m 52.27^s

−60° 07′ 04.0″

6.46

−5.05

6520

WN7 + A

in Collinder 228; Wolf–Rayet star, V_max = 6.46^m, V_min = 6.49^m, P = 4.76 d; one of the most luminous stars known

HD 52622

52622

33577

06^h 58^m 36.39^s

−56° 23′ 41.2″

6.46

1.46

326

F2II

suspected variable

HD 54967

54967

34350

07^h 07^m 16.28^s

−59° 42′ 59.2″

6.46

−1.79

1455

B3V

HD 93738

93738

52815

10^h 47^m 53.55^s

−64° 15′ 46.3″

6.46

0.67

469

B9.5V

in IC 2602

HD 49219

49219

32269

06^h 44^m 12.81^s

−54° 41′ 43.9″

6.47

−0.30

736

B5/B6V

variable star, ΔV = 0.011^m, P = 1.60 d

HD 70267

70267

40655

08^h 17^m 55.79^s

−59° 10′ 00.3″

6.47

2.01

254

F5V

V487 Car

V487

84809

47893

09^h 45^m 40.64^s

−57° 11′ 09.8″

6.47

−0.66

869

B8III/IV

α² CVn variable

HD 93695

93695

52806

10^h 47^m 44.34^s

−59° 52′ 30.9″

6.47

−1.41

1230

B5Vvar

HD 95122

95122

53556

10^h 57^m 20.22^s

−69° 02′ 17.0″

6.48

−0.55

832

B7V

suspected variable

HD 92399

92399

52103

10^h 38^m 45.39^s

−59° 15′ 44.7″

6.50

−1.82

1502

B4/B5III/IV

HD 96248

V414

96248

54179

11^h 04^m 57.57^s

−59° 51′ 32.0″

6.58

3700

B1Iab

α Cyg variable, V_max = 6.53^m, V_min = 6.62^m, P = 8.52 d

HD 57853

57853

35564

07^h 20^m 21.43^s

−52° 18′ 31.91″

6.63

113

F9V

component of the HIP 35564 system

QX Car

QX

86118

48589

09^h 54^m 33.88^s

−58° 25′ 16.6″

6.64

1610

B2V

Algol variable, V_max = 6.6^m, V_min = 7.21^m, P = 4.48 d

HD 96446

V430

96446

54266

11^h 06^m 05.82^s

−59° 56′ 59.6″

6.68

1540

B2k

β Cep variable, ΔV = 0.03^m

HD 53143

53143

33690

06^h 59^m 59.66^s

−61° 20′ 10.3″

6.68

59.74

G9V

has a circumstellar disk

VY Car

VY

93203

52538

10^h 44^m 32.69^s

−57° 33′ 55.3″

6.91

9100

F7Iab/Ib

classical Cepheid, V_max = 6.91^m, V_min = 8.00^m, P = 18.89 d

AG Car

AG

94910

53461

10^h 56^m 11.58^s

−60° 27′ 12.8″

6.96

17000

B2-3Ib/WN11

luminous blue variable, V_max = 5.7^m, V_min = 8.3^m, P = 371.4 d

BO Car

BO

93420

10^h 45^m 50.63^s

−59° 29′ 19.5″

7.18

M4Iab:

semiregular variable, V_max = 7.15^m, V_min = 7.95^m, P = 130.7 d

HD 93403

93403

52628

10^h 45^m 44.12^s

−59° 24′ 28.1″

7.30

2670

O5.5I+O7V

binary star

HD 93129A

93129A

10^h 43^m 57.46^s

−59° 32′ 51.2″

7.31

7500

O2If*+O3.5

in Trumpler 14; binary star; primary is one of the most luminous stars known

V Car

V

72275

41588

08^h 28^m 43.70^s

−60° 07′ 21.3″

7.31

5600

G2Iab:

classical Cepheid, V_max = 7.08^m, V_min = 7.82^m, P = 6.70 d

HD 93843

93843

10^h 48^m 37.78^s

−60° 13′ 25.5″

7.33

O5III(f)v

irregular variable, V_max = 7.31^m, V_min = 7.35^m

HD 95086

95086

53524

10^h 57^m 03.0^s

−68° 40′ 02″

7.36

295

A8III

has a planet (b)

HD 93250

93250

52558

10^h 44^m 45.03^s

−59° 33′ 54.7″

7.50

7500

O4IIIfc

in Trumpler 16; suspected variable

HR Car

HR

90177

50843

10^h 22^m 53.84^s

−59° 37′ 28.4″

7.57

17700

B3Iaep

luminous blue variable, V_max = 6.8^m, V_min = 8.80^m

WR 40

V385

96548

54283

11^h 06^m 17.20^s

−65° 30′ 35.2″

7.70

5900

WN8h

Wolf–Rayet star and rotating ellipsoidal variable, ΔV = 0.04^m, P = 4.76 d; one of the most luminous stars known

HD 93205

V560

93205

10^h 44^m 33.74^s

−59° 44′ 15.5″

7.75

7500

O3.5V((f+))

in Trumpler 16; rotating ellipsoidal variable, V_max = 7.74^m, V_min = 7.76^m, P = 6.08 d

IW Car

IW

82084
82085

09^h 26^m 53.30^s

−63° 37′ 48.9″

7.90

A4Iab/II:

RV Tau variable, V_max = 7.77^m, V_min = 9.10^m, P = 143.6 d

HD 65216

65216

38558

07^h 53^m 41.3^s

−63° 38′ 50.4″

7.98

112

G5V

has two planets (b & c)

HD 97152

V431

97152

54574

11^h 10^m 04.08^s

−60° 58′ 45.0″

8.07

4000

WC7+O7V

Wolf–Rayet star; eclipsing binary, V_max = 7.97^m, V_min = 8.08^m, P = 1.62 d

HD 63765

63765

38041

07^h 47^m 49.72^s

−54° 15′ 50.9″

8.10

5.53

106

G9V

Tapecue; has a planet (b)

Y Car

Y

91565

51653

10^h 33^m 10.85^s

−58° 29′ 55.1″

8.16

3050

F2

double-mode Cepheid, V_max = 7.53^m, V_min = 8.48^m, P = 3.64 d

HD 51608

51608

33229

06^h 54^m 51^s

−55° 15′ 34″

8.17

114

K0IV

has two planets (b & c)

HD 85628 A

85628

09^h 50^m 19.2^s

−66° 06′ 50″

8.19

559

A3V

has a planet (b)

YZ Car

YZ

90912

51262

10^h 28^m 16.85^s

−59° 21′ 00.7″

8.24

5900

G5

classical Cepheid, V_max = 8.24^m, V_min = 9.08^m, P = 18.17 d

WR 16

V396

86161

48617

09^h 54^m 52.90^s

−57° 43′ 38.3″

8.32

WN8h

rotating ellipsoidal variable, ΔV = 0.06^m; one of the most luminous stars known

EM Car

EM

97484

11^h 12^m 04.51^s

−61° 05′ 42.9″

8.52

O8V

Algol variable

RT Car

RT

303310

52562

10^h 44^m 47.15^s

−59° 24′ 48.1″

8.55

1430

M2Iab:

possibly in Trumpler 15; irregular variable, V_max = 8.2^m, V_min = 9.9^m, one of the largest stars known

HD 85567

V596

85567

48269

09^h 50^m 28.54^s

−60° 58′ 03.0″

8.57

6900

B2

FS CMa variable, V_max = 8.44^m, V_min = 8.75^m

UX Car

UX

91039

51338

10^h 29^m 11.24^s

−57° 36′ 48.3″

8.62

2530

F2II

classical Cepheid, V_max = 7.81^m, V_min = 8.67^m, P = 3.68 d

XZ Car

XZ

305996

54101

11^h 04^m 13.47^s

−60° 58′ 47.7″

8.67

B2:pe

classical Cepheid, V_max = 8.05^m, V_min = 9.12^m, P = 16.65 d

GG Car

GG

94878

53444

10^h 55^m 58.92^s

−60° 23′ 33.4″

8.70

B0/2eq

Be star and re-radiating binary system, V_max = 8.44^m, V_min = 9.08^m, P = 31.03 d

V403 Car

V403

10^h 35^m 40.67^s

−58° 12′ 44.6″

8.74

8400

B1III

in NGC 3293; β Cep variable, ΔV = 0.033^m, P = 0.25 d

Tr 16-104

V572

10^h 44^m 47.31^s

−59° 43′ 53.2″

8.75

7500

O7V((f))+
O9.5V+
B0.2IV

in Trumpler 16; Algol variable, V_max = 8.66^m, V_min = 9.07^m, P = 2.15 d

V348 Car

V348

90707

10^h 29^m 59.00^s

−57° 40′ 32.8″

8.78

B1III

β Lyr variable, V_max = 8.55^m, V_min = 8.93^m, P = 5.56 d

WR 25

93162

10^h 44^m 10.34^s

−59° 43′ 11.4″

8.80

7500

O2.5If*/WN6

in Trumpler 16; Wolf–Rayet star; one of the most luminous stars known

HD 60435

V409

60435

36537

07^h 30^m 56.99^s

−57° 59′ 28.2″

8.89

739

Ap...

rapidly oscillating Ap star

WR 23

92809

52331

10^h 41^m 38.32^s

−58° 46′ 18.7″

9.03

3400

WC6

Wolf–Rayet star

HD 92024

V381

92024

10^h 36^m 08.31^s

−58° 13′ 04.77″

9.04

8400

B1III

in NGC 3293; β Cep variable, V_max = 9.04^m, V_min = 9.06^m, P = 0.17 d

GH Car

GH

306077

54621

11^h 10^m 44.59^s

−60° 45′ 01.0″

9.20

G0

classical Cepheid, V_max = 9^m, V_min = 9.35^m, P = 5.73 d

WZ Car

WZ

94777

53397

10^h 55^m 18.73^s

−60° 56′ 24.0″

9.37

4700

F8

classical Cepheid, V_max = 8.63^m, V_min = 9.88^m, P = 23.02 d

CPD -59° 2635

V731

10^h 45^m 12.72^s

−59° 44′ 46.2″

9.43

7500

O8V+O9.5V

in Trumpler 16; Algol variable, V_max = 9.27^m, V_min = 9.78^m, P = 2.30 d

V392 Car

V392

07^h 58^m 10.47^s

−60° 51′ 57.5″

9.49

A2Vp...

in NGC 2516; Algol and α² CVn variable, V_max = 9.49^m, V_min = 9.67^m

XY Car

XY

308149

53945

11^h 02^m 16.07^s

−64° 15′ 46.5″

9.49

G5

classical Cepheid, V_max = 8.82^m, V_min = 9.77^m, P = 12.43 d

HD 87643

V640

87643

10^h 04^m 30.29^s

−58° 39′ 52.1″

9.50

B2e

Orion variable, V_max = 7.4^m, V_min = 9.8^m

CPD -59 2628

V573

10^h 45^m 08.23^s

−59° 40′ 49.5″

9.52

7500

O9.5V+B0.3V

in Trumpler 16; Algol variable

HD 90657

V398

90657

51109

10^h 26^m 31.41^s

−58° 38′ 26.2″

9.69

3500

WN5+O4-6

Wolf–Rayet star; eclipsing binary, ΔV = 0.035^m

GL Car

GL

306168

11^h 14^m 39.84^s

−60° 39′ 36.3″

9.70

B3:V

Algol variable

DW Car

DW

305543

10^h 43^m 10.07^s

−60° 02′ 11.7″

9.85

B2:pe

in Collinder 228; Algol variable

SS73 17

V648

10^h 11^m 02.95^s

−57° 48′ 13.9″

9.99

M3pe+OB

Z And variable, V_max = 9.6^m, V_min = 10.0^m, P = 520 d

CPD -57 2874

10^h 15^m 21.97^s

−57° 51′ 42.7″

10.16

sgB1[e]

B[e] star

GZ Car

GZ

302719

50615

10^h 20^m 20.37^s

−59° 22′ 35.8″

10.20

2400

G5

double-mode Cepheid, V_max = 9.98^m, V_min = 10.47^m, P = 4.16 d

HH Car

HH

303503

10^h 53^m 36.47^s

−59° 27′ 18.2″

10.31

B

Algol variable, V_max = 10.3^m, V_min = 10.82^m, P = 3.23 d

EY Car

EY

52380

10^h 42^m 23.03^s

−61° 09′ 57.3″

10.35

B2:pe

double-mode Cepheid, V_max = 10.01^m, V_min = 10.56^m, P = 2.88 d

HD 307938

V557

307938

10^h 42^m 41.52^s

−64° 21′ 04.4″

10.57

G2V

BY Dra variable, ΔV = 0.21^m

WR 18

V500

89358

50368

10^h 17^m 02.27^s

−57° 54′ 47.9″

10.6

6300

WN4-s

Wolf–Rayet star

HD 94546

V428

94546

53274

10^h 53^m 44.82^s

−59° 30′ 46.7″

10.7

WN4+O8V

Wolf–Rayet star; eclipsing binary, ΔV = 0.05^m

He 3-519

10^h 53^m 59.59^s

−60° 26′ 44.3″

10.85

WN11

Wolf–Rayet star, V_max = 10.6^m, V_min = 11.0^m

NGC 3603-A1

97950A

11^h 15^m 07.31^s

−61° 15′ 38.4″

11.12

20000

WN6ha+O3V

in NGC 3603; Algol variable, ΔV = 0.45^m, P = 3.77 d both components among the most luminous and massive stars known

CR Car

CR

10^h 32^m 54.07^s

−58° 31′ 15.5″

11.30

B2:pe

classical Cepheid, V_max = 11.3^m, V_min = 11.89^m, P = 9.76 d

NGC 3603-B

97950B

11^h 15^m 07.41^s

−61° 15′ 38.6″

11.33

WN6h+abs

one of the most luminous and most massive stars known

Innes' star

11^h 16^m 00.21^s

−57° 32′ 51.6″

11.52

41.31

M3.5

has a planet

QU Car

QU

310376

54226

11^h 05^m 42.49^s

−68° 37′ 58.2″

11.54

1290

B+...

V Sge variable, V_max = 10.9^m, V_min = 11.7^m, P = 0.45 d

WR 30

V541

94305

10^h 51^m 06.01^s

−62° 17′ 01.7″

11.73

WC6+O7.5V

Algol variable, ΔV = 0.09^m

Wray 15-751

V432

11^h 08^m 40.06^s

−60° 42′ 51.7″

11.79

WR:

luminous blue variable, V_max = 10.7^m, V_min = 12.43^m

NGC 3603-C

97950C

11^h 15^m 07.59^s

−61° 15′ 18.0″

11.89

WN6h+abs

spectroscopic binary

FO 15

V662

10^h 45^m 36.32^s

−59° 48′ 23.2″

12.09

7500

O5.5V+O9.5V

in Trumpler 16; Algol variable, V_max = 12.09^m, V_min = 12.7^m, P = 1.41 d

Sher 25

11^h 15^m 07.8^s

−61° 15′ 17″

12.27

B1.5Iab

in NGC 3603; potential supernova progenitor

WR 30a

V574

10^h 51^m 38.93^s

−60° 56′ 35.2″

12.73

WR+...

Algol variable, ΔV = 0.05^m

GJ 1128

09^h 42^m 46.356^s

−68° 53′ 06.04″

12.78

M4.0V

He 2-38

V366

09^h 54^m 43.29^s

−57° 18′ 52.4″

12.92

M5-7.5

Mira and Z And variable, V_max = 12.1^m, V_min = 14.4^m, P = 433 d

BPM 6502

V727

10^h 44^m 10.23^s

−69° 18′ 18.0″

13.09

DA2.2+M

re-radiating binary system

WR 20a

V712

10^h 23^m 58.00^s

−57° 45′ 49.0″

13.5

O3If*/WN6+
O3If*/WN6

in Westerlund 2; Algol variable

LHS 288

10^h 44^m 21.32^s

−61° 12′ 38.4″

13.92

15.602

M4

OGLE-TR-113

V752

10^h 52^m 24.4^s

−61° 26′ 48.5″

14.42

1800

K

has a transiting planet (b)

MTT 68

11^h 14^m 59.50^s

−61° 14′ 33.89″

14.72

−6.4

25,000

O2If*

rare O2If* type, along with HD 93129A

2S 0921-630

V395

09^h 22^m 35.20^s

−63° 17′ 38.5″

15.3

K0IIIe

low-mass X-ray binary

OGLE-TR-123

V816

11^h 06^m 51.1^s

−61° 11′ 10.5″

15.47

FV+MV

possibly has a transiting planet

OGLE-TR-111

V759

10^h 53^m 17.9^s

−61° 24′ 20.3″

15.55

5000

G

has a transiting planet (b) and
a possible second planet

OGLE-TR-132

V742

10^h 50^m 34.7^s

−61° 57′ 25.9″

15.72

7110

F

has a transiting planet (b)

OY Car

OY

10^h 06^m 22.07^s

−70° 14′ 04.6″

16.2

277

M5/M6:...

SU UMa variable and eclipsing binary, V_max = 11.2^m, V_min = 16.2^m, P = 0.063 d

OGLE-TR-182

11^h 09^m 18.73^s

−61° 05′ 42.93″

16.84

12700

G

has a transiting planet (b)

OGLE-TR-211

10^h 40^m 14.39^s

−62° 27′ 20.2″

5300

F

has a transiting planet (b)

OGLE-TR-122

V817

11^h 06^m 52.0^s

−60° 51′ 45.7″

has a transiting brown dwarf

OGLE2-TR-L9

11^h 07^m 55^s

−61° 08′ 46″

2935

F3

has a transiting planet (b)

1E 1048.1-5937

10^h 50^m 08.93^s

−59° 53′ 19.9″

Be

anomalous X-ray pulsar

DENIS J081730.0-615520

08^h 17^m 30.01^s

−61° 55′ 15.8″

16.1

T6

brown dwarf

PSR J1048-5832

10^h 48^m 12.20^s

−58° 32′ 05.8″

pulsar

PSR J1119-6127

11^h 19^m 14.30^s

−61° 27′ 49.5″

pulsar

Table legend:

• Name = Proper name
• B = Bayer designation
• F or/and G. = Flamsteed designation or Gould designation
• Var = Variable star designation
• HD = Henry Draper Catalogue designation number
• HIP = Hipparcos Catalogue designation number
• RA = Right ascension for the Epoch/Equinox J2000.0
• Dec = Declination for the Epoch/Equinox J2000.0

• vis. mag. = visual magnitude (m or m_v), also known as apparent magnitude
• abs. mag. = absolute magnitude (M_v)
• Dist. (ly) = Distance in light-years from Earth
• Sp. class = Spectral class of the star in the stellar classification system
• Notes = Common name(s) or alternate name(s); comments; notable properties [for example: multiple star status, range of variability if it is a variable star, exoplanets, etc.]

Notes

^ Gray, R. O.; Garrison, R. F. (1989-02-01). "The Early F-Type Stars: Refined Classification, Confrontation with Stroemgren Photometry, and the Effects of Rotation". The Astrophysical Journal Supplement Series. 69: 301. Bibcode:1989ApJS...69..301G. doi:10.1086/191315. ISSN 0067-0049.
^ Lopez-Cruz, O.; Garrison, R. F. (1993-01-01). "A Spectroscopic Study of High Galactic Latitude F Supergiant Stars". Luminous High-Latitude Stars. 45: 59. Bibcode:1993ASPC...45...59L.
^ Kunitzsch, P., & Smart, T. (2006). A Dictionary of Modern star Names: A Short Guide to 254 Star Names and Their Derivations (2nd rev. ed.). Cambridge, MA: Sky Pub. p. 25. ISBN 978-1-931559-44-7.{{cite book}}: CS1 maint: multiple names: authors list (link)
^ Gray, R. O.; Corbally, C. J.; Garrison, R. F.; McFadden, M. T.; Bubar, E. J.; McGahee, C. E.; O'Donoghue, A. A.; Knox, E. R. (July 2006). "Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 parsecs: The Southern Sample". The Astronomical Journal. 132 (1): 161–170. arXiv:astro-ph/0603770. doi:10.1086/504637. ISSN 0004-6256.

References

ESA (1997). "The Hipparcos and Tycho Catalogues". Retrieved 2006-12-26.
Kostjuk, N. D. (2002). "HD-DM-GC-HR-HIP-Bayer-Flamsteed Cross Index". Retrieved 2006-12-26.
Roman, N. G. (1987). "Identification of a Constellation from a Position". Retrieved 2006-12-26.
"SIMBAD Astronomical Database". Centre de Données astronomiques de Strasbourg. Retrieved 2007-01-02.
Gould, B. A. "Uranometria Argentina". Reprinted and updated by Pilcher, F. Archived from the original on 2012-02-27. Retrieved 2010-07-19.
Samus, N. N.; Durlevich, O. V.; et al. (2004). "Combined General Catalogue of Variable Stars (GCVS4.2)". Retrieved 2012-04-08.
Samus, N. N.; Durlevich, O. V.; et al. (2012). "General Catalog of Variable Stars (GCVS database, version 2012Feb)". Retrieved 2012-04-08.
"AAVSO Website". American Association of Variable Star Observers. Retrieved 9 March 2014.

[1] Gray, R. O.; Garrison, R. F. (1989-02-01). "The Early F-Type Stars: Refined Classification, Confrontation with Stroemgren Photometry, and the Effects of Rotation". The Astrophysical Journal Supplement Series. 69: 301. Bibcode:1989ApJS...69..301G. doi:10.1086/191315. ISSN 0067-0049.

[2] Lopez-Cruz, O.; Garrison, R. F. (1993-01-01). "A Spectroscopic Study of High Galactic Latitude F Supergiant Stars". Luminous High-Latitude Stars. 45: 59. Bibcode:1993ASPC...45...59L.

[3] Kunitzsch, P., & Smart, T. (2006). A Dictionary of Modern star Names: A Short Guide to 254 Star Names and Their Derivations (2nd rev. ed.). Cambridge, MA: Sky Pub. p. 25. ISBN 978-1-931559-44-7.{{cite book}}: CS1 maint: multiple names: authors list (link)

[4] Gray, R. O.; Corbally, C. J.; Garrison, R. F.; McFadden, M. T.; Bubar, E. J.; McGahee, C. E.; O'Donoghue, A. A.; Knox, E. R. (July 2006). "Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 parsecs: The Southern Sample". The Astronomical Journal. 132 (1): 161–170. arXiv:astro-ph/0603770. doi:10.1086/504637. ISSN 0004-6256.

[1]

[2]

[3]

[4]

See also

Notes

References