List of coolest stars
Appearance
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This is a list of coolest stars and brown dwarfs discovered, arranged by decreasing temperature. The stars with temperatures lower than 2,000 K are included.
Kirkpatrick et al. 2021[1] has a more complete list of nearby objects with a temperature below 2,400 K. Objects with a temperature below 500 K from this paper were included in this list.
List
[edit]Star name | Temperature
(K) |
Spectral type | Distance (light years) | Notes |
---|---|---|---|---|
WISE 0855–0714 | 285 | Y4 | 7.426±0.039 | [2] |
WISE 0336-0143B[3] | 295±10[4] | Y1? | 32.7[1] | spectral type is not yet published, but should be around Y1 if we assume MIRI F480M is similar to W2 and by using Figure 13 from Kirkpatrick et al. 2012[5] Might be a later spectral type. |
WISEA 0830+2837 | 300-350[6] | >Y1[1] | 26.87[1] | uncertain parallax and spectral type is an estimate |
CWISEP 0238-1332 | 367±79[1] | >Y1 | 58.66 | uncertain parallax and spectral type is an estimate |
CWISEP 0402-2651 | 367±79[1] | >Y1 | 39.53 | uncertain parallax and spectral type is an estimate |
WISEU 0503-5648[1] | 367±79 | >Y1 | 33.18 | spectral type is an estimate |
CWISEP 0940+5233[1] | 367±79 | >Y1 | 43.49 | uncertain parallax and spectral type is an estimate |
WISEA 1257+7153[1] | 367±79 | >Y1 | 54.18 | spectral type is an estimate |
CWISEP J1446−2317[1] | 367±79 | >Y1 | 37.75 | uncertain parallax and spectral type is an estimate |
WISEA 1930-2059[1] | 367±79 | >Y1 | 30.67 | spectral type is an estimate |
CWISEP 1935-1546[1] | 367±79 | >Y1 | 47.06 | spectral type is an estimate |
CWISEP 2230+2549[1] | 367±79 | >Y1 | 52.44 | uncertain parallax and spectral type is an estimate |
CWISEP 2256+4002[1] | 367±79 | >Y1 | 32.04 | spectral type is an estimate |
WISE 0825+2805[1] | 376±88 | Y0.5 | 21.37 | |
WD 0806-661B[1] | 377±88 | Y1 | 62.80 | spectral type is an estimate |
WISE 0350-5658[1] | 388±88 | Y1 | 18.49 | |
WISEA 2354+0240[1] | 388±88 | Y1 | 24.97 | |
WISE 2209+2711[1] | 389±88 | Y0: | 20.17 | |
WISE 0647-6232[1] | 393±88 | Y1 | 32.78 | |
WISEPA 1541-2250[1] | 395±88 | Y1 | 19.54 | |
WISE 1828+2650 | 406±88[1] | Y2V[7] | 32.5 | Temperature could be lower. If it is a binary, its components could be as cold as about 275-350 K.[8] |
WISE 0535-7500[1] | 410±88 | >=Y1: | 47.48 | |
WISE 1405+5534 | 411±88[1] | Y0.5(pec?)[1] | 20.62 | |
CWISEP 0321+6932[1] | 412±79 | Y0.5 | 47.61 | spectral type is an estimate |
WISE 1639-6847[1] | 412±88 | Y0pec | 14.85 | |
CWISEP 2356-4814[1] | 412±79 | Y0.5 | 56.62 | spectral type is an estimate |
WISE 0336-0143A[3] | 440±24[9] | Y0[1] | 32.7[1] | |
WISEPA 1738+2732[1] | 450±88 | Y0 | 24.92 | |
WISEPA 0410+1502[1] | 451±88 | Y0 | 21.56 | |
WISE 2220-3628[1] | 452±88 | Y0 | 34.15 | |
WISE 1534-1043 | 453±77[10] | sdY? | 53 | possibly halo brown dwarf |
WISE 1206+8401[1] | 454±88 | Y0 | 38.51 | |
WISE 0146+4234B[1] | 460±79 | Y0 | 63.09 | |
WISEA 0302-5817[1] | 460±79 | Y0: | 54.45 | |
CWISEP 0634+5049[1] | 460±79 | Y0 | 52.61 | spectral type is an estimate |
CWISEP 0859+5349[1] | 460±79 | Y0 | 60.62 | spectral type is an estimate |
CWISE 0925-4720[1] | 460±79 | Y0 | 34.96 | spectral type is an estimate |
CWISEP 0938+0634[1] | 460±79 | Y0 | 61.31 | uncertain parallax and spectral type is an estimate |
CWISEP J1047+5457[1] | 460±79 | Y0 | 43.37 | spectral type is an estimate |
CWISE 1121-6232[1] | 460±79 | Y0 | 33.69 | spectral type is an estimate |
WISEA 1141-3326[1] | 460±79 | Y0 | 31.36 | |
WISE 1217+1626 B | 460±79[1] | Y0-0.5 | 33 | |
CWISE 1531-3306[1] | 460±79 | Y0 | 55.37 | spectral type is an estimate |
WISENF 1936+0408[1] | 460±79 | Y0 | 28.64 | spectral type is an estimate |
CWISEP 2011-4812[1] | 460±79 | Y0 | 45.94 | spectral type is an estimate |
WISEA 2243-1458[1] | 460±79 | Y0 | 47,75 | spectral type is an estimate |
WISE 1112-3857[1] | 461±88 | T9 | 31.79 | |
WISE 0734-7157[1] | 462±88 | Y0 | 43.78 | |
WISE 0713-2917[1] | 464±88 | Y0 | 29.84 | |
WISEPC 2056+1459[1] | 464±88 | Y0 | 23.16 | |
WISE 0304-2705[1] | 465±88 | Y0~pec | 44.62 | |
WISE 0359-5401 | 467+16 −18[11] |
Y0[1] | 44.31[1] | |
WISE 0943+3607[1] | 468±88 | T9.5 | 33.59 | |
WISE 0833+0052[1] | 472±88 | (sd)T9 | 40.92 | possible subdwarf |
WISE 1542+2230[1] | 472±88 | T9.5 | 38.69 | |
WISE 0811-8051[1] | 479±88 | T9.5: | 32.91 | |
WISEPA 2134-7137[1] | 481±88 | T9~pec | 29.73 | possible subdwarf |
WISE 2212-6931[1] | 487±88 | T9 | 40.47 | |
WISEPA 0751-7634[1] | 492±88 | T9 | 33.32 | |
WISE 0335+4310[1] | 492±88 | T9 | 38.46 | |
2MASS 0939-2448 A/B | 650[12] | T8 | 17.4±0.4 | |
54 Piscium B | 810 ± 50 | T7.5V | 36.32±0.02 | [13] |
2M 1237+6526 | 850[14] | T6.5 | 46 | |
2MASS J0348−6022 | 880 | T7[15] | 27.2 | |
GD 165 B | 1,755[16] | L4[17] | 109 | |
S Cassiopeiae | 1,800[18] | S3,4–S5,8 | 3,100±300 | |
RW Leonis Minoris | 1,800[19] | C4,3[20] | 1,053[21] | |
V384 Persei | 1,820[22] | N | ||
DENIS-P J1058.7−1548 | 1,850[23] | L3 | 49 | |
T Draconis | 1,850[22] | C6,2e | ||
V346 Puppis | 1,875[22] | C | ||
2MASS J0523-1403 | 1,939[24] | L2.5V | 41.62 | The coolest main sequence star known as of 2023. |
S Aurigae | 1,940[22] | C-N5+ | ||
V1426 Cygni | 1,975[22] | C7,2e |
See also
[edit]
References
[edit]- ^ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag ah ai aj ak al am an ao ap aq ar as at au av aw ax ay az ba bb bc bd be bf bg bh bi bj bk Kirkpatrick, J. Davy; Gelino, Christopher R.; Faherty, Jacqueline K.; Meisner, Aaron M.; Caselden, Dan; Schneider, Adam C.; Marocco, Federico; Cayago, Alfred J.; Smart, R. L.; Eisenhardt, Peter R.; Kuchner, Marc J.; Wright, Edward L.; Cushing, Michael C.; Allers, Katelyn N.; Gagliuffi, Daniella C. Bardalez (2021-03-01). "The Field Substellar Mass Function Based on the Full-sky 20-pc Census of 525 L, T, and Y Dwarfs". The Astrophysical Journal Supplement Series. 253 (1): 7. arXiv:2011.11616. Bibcode:2021ApJS..253....7K. doi:10.3847/1538-4365/abd107. ISSN 0067-0049. S2CID 227126954.
- ^ Luhman, K. L.; Tremblin, P.; Alves de Oliveira, C.; Birkmann, S. M.; Baraffe, I.; Chabrier, G.; Manjavacas, E.; Parker, R. J.; Valenti, J. (2023-12-05). "JWST/NIRSpec Observations of the Coldest Known Brown Dwarf*". The Astronomical Journal. 167 (1): 5. arXiv:2311.17316. doi:10.3847/1538-3881/ad0b72. ISSN 0004-6256.
- ^ a b Calissendorff, Per; De Furio, Matthew; Meyer, Michael; Albert, Loïc; Aganze, Christian; Ali-Dib, Mohamad; Bardalez Gagliuffi, Daniella C.; Baron, Frederique; Beichman, Charles A.; Burgasser, Adam J.; Cushing, Michael C.; Faherty, Jacqueline Kelly; Fontanive, Clémence; Gelino, Christopher R.; Gizis, John E. (2023-04-01). "JWST/NIRCam Discovery of the First Y+Y Brown Dwarf Binary: WISE J033605.05-014350.4". The Astrophysical Journal. 947 (2): L30. arXiv:2303.16923. Bibcode:2023ApJ...947L..30C. doi:10.3847/2041-8213/acc86d. ISSN 0004-637X.
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- ^ Beichman, Charles A.; Gelino, Christopher R.; Kirkpatrick, J. Davy; Barman, Travis S.; Marsh, Kenneth A.; Cushing, Michael C.; Wright, E. L. (2013-01-29). "The Coldest Brown Dwarf (Or Free Floating Planet)?: The Y Dwarf WISE 1828+2650". The Astrophysical Journal. 764 (1): 101. arXiv:1301.1669. Bibcode:2013ApJ...764..101B. doi:10.1088/0004-637X/764/1/101. ISSN 0004-637X. S2CID 118575478.
- ^ Cushing, Michael C.; Schneider, Adam C.; Kirkpatrick, J. Davy; Morley, Caroline V.; Marley, Mark S.; Gelino, Christopher R.; Mace, Gregory N.; Wright, Edward L.; Eisenhardt, Peter R.; Skrutskie, Michael F.; Marsh, Kenneth A. (2021-10-01). "An Improved Near-infrared Spectrum of the Archetype Y Dwarf WISEP J182831.08+265037.8". The Astrophysical Journal. 920 (1): 20. arXiv:2107.00506. Bibcode:2021ApJ...920...20C. doi:10.3847/1538-4357/ac12cb. ISSN 0004-637X.
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- ^ Leggett, Sandy K.; Cushing, Michael C.; Saumon, Didier; Marley, Mark S.; Roellig, Thomas L.; Warren, Stephen J.; Burningham, Ben; Jones, Hugh R. A.; Kirkpatrick, J. Davy; Lodieu, Nicolas; Lucas, Philip W.; Mainzer, Amy K.; Martín, Eduardo L.; McCaughrean, Mark J.; Pinfield, David J.; Sloan, Gregory C.; Smart, Richard L.; Tamura, Motohide; Van Cleve, Jeffrey E. (2009). "The Physical Properties of Four ~600 K T Dwarfs". The Astrophysical Journal. 695 (2): 1517–1526. arXiv:0901.4093. Bibcode:2009ApJ...695.1517L. doi:10.1088/0004-637X/695/2/1517. S2CID 44050900.
- ^ Luhman, K. L.; Patten, B. M.; Marengo, M.; Schuster, M. T.; Hora, J. L.; Ellis, R. G.; Stauffer, J. R.; Sonnett, S. M.; Winston, E.; Gutermuth, R. A.; Megeath, S. T.; Backman, D. E.; Henry, T. J.; Werner, M. W.; Fazio, G. G. (January 2007). "Discovery of Two T Dwarf Companions with the Spitzer Space Telescope". The Astrophysical Journal. 654 (1): 570–579. arXiv:astro-ph/0609464. Bibcode:2007ApJ...654..570L. doi:10.1086/509073. ISSN 0004-637X.
- ^ Liebert & Burgasser (2007). "On the Nature of the Unique Hα-emitting T Dwarf 2MASS J12373919+6526148". Astronomy & Astrophysics. 655 (1): 522–527. arXiv:astro-ph/0609793. Bibcode:2007ApJ...655..522L. doi:10.1086/509882. S2CID 18852560.
- ^ Tannock, Megan E.; Metchev, Stanimir; Heinze, Aren; Miles-Páez, Paulo A.; Gagné, Jonathan; Burgasser, Adam; Marley, Mark S.; Apai, Dániel; Suárez, Genaro; Plavchan, Peter (2021-05-01). "Weather on Other Worlds. V. The Three Most Rapidly Rotating Ultra-Cool Dwarfs". The Astronomical Journal. 161 (5): 224. arXiv:2103.01990. Bibcode:2021AJ....161..224T. doi:10.3847/1538-3881/abeb67. ISSN 0004-6256. S2CID 232105126.
- ^ Filippazzo, Joseph C.; Rice, Emily L.; Faherty, Jacqueline; Cruz, Kelle L.; Van Gordon, Mollie M.; Looper, Dagny L. (2015-09-10). "Fundamental Parameters and Spectral Energy Distributions of Young and Field Age Objects with Masses Spanning the Stellar to Planetary Regime". The Astrophysical Journal. 810 (2): 158. arXiv:1508.01767. Bibcode:2015ApJ...810..158F. doi:10.1088/0004-637X/810/2/158. ISSN 1538-4357. S2CID 89611607.
- ^ Kirkpatrick, J. Davy; Reid, I. Neill; Liebert, James; Cutri, Roc M.; Nelson, Brant; Beichman, Charles A.; Dahn, Conard C.; Monet, David G.; Gizis, John E.; Skrutskie, Michael F. (1999-07-01). "Dwarfs Cooler than M: The Definition of Spectral Type L Using Discoveries from the 2 Micron All-Sky Survey (2MASS)". The Astrophysical Journal. 519 (2): 802–833. Bibcode:1999ApJ...519..802K. doi:10.1086/307414. ISSN 0004-637X. S2CID 73569208.
- ^ Ramstedt, S.; Olofsson, H. (2014-06-01). "The 12CO/13CO ratio in AGB stars of different chemical type - Connection to the 12C/13C ratio and the evolution along the AGB". Astronomy & Astrophysics. 566: A145. arXiv:1405.6404. doi:10.1051/0004-6361/201423721. ISSN 0004-6361.
- ^ Ramstedt, S.; Olofsson, H. (2014-06-01). "The 12CO/13CO ratio in AGB stars of different chemical type - Connection to the 12C/13C ratio and the evolution along the AGB". Astronomy & Astrophysics. 566: A145. arXiv:1405.6404. doi:10.1051/0004-6361/201423721. ISSN 0004-6361.
- ^ Cohen, M. (1979-03-01). "Circumstellar envelopes and the evolution of carbon stars". Monthly Notices of the Royal Astronomical Society. 186 (4): 837–852. Bibcode:1979MNRAS.186..837C. doi:10.1093/mnras/186.4.837. ISSN 0035-8711.
- ^ Bailer-Jones, C. A. L.; Rybizki, J.; Fouesneau, M.; Demleitner, M.; Andrae, R. (2021-03-01). "Estimating distances from parallaxes. V: Geometric and photogeometric distances to 1.47 billion stars in Gaia Early Data Release 3". The Astronomical Journal. 161 (3): 147. arXiv:2012.05220. Bibcode:2021AJ....161..147B. doi:10.3847/1538-3881/abd806. ISSN 0004-6256. Data about this star can be seen here.
- ^ a b c d e Bergeat, J.; Chevallier, L. (2005). "The mass loss of C-rich giants". Astronomy and Astrophysics. 429: 235–246. arXiv:astro-ph/0601366. Bibcode:2005A&A...429..235B. doi:10.1051/0004-6361:20041280. S2CID 56424665.
- ^ Heinze, Aren N.; Metchev, Stanimir; Apai, Daniel; Flateau, Davin; Kurtev, Radostin; Marley, Mark; Radigan, Jacqueline; Burgasser, Adam J.; Artigau, Étienne; Plavchan, Peter (2013-04-08). "Weather on Other Worlds I: Detection of Periodic Variability in the L3 Dwarf DENIS-P J1058.7-1548 with Precise Multi-Wavelength Photometry". The Astrophysical Journal. 767 (2): 173. arXiv:1303.2948. Bibcode:2013ApJ...767..173H. doi:10.1088/0004-637X/767/2/173. ISSN 0004-637X. S2CID 29406867.
- ^ Filippazzo, Joseph C.; Rice, Emily L.; Faherty, Jacqueline; Cruz, Kelle L.; Van Gordon, Mollie M.; Looper, Dagny L. (2015-09-10). "Fundamental Parameters and Spectral Energy Distributions of Young and Field Age Objects with Masses Spanning the Stellar to Planetary Regime". The Astrophysical Journal. 810 (2): 158. arXiv:1508.01767. Bibcode:2015ApJ...810..158F. doi:10.1088/0004-637X/810/2/158. ISSN 1538-4357.