HD 225218
Appearance
(Redirected from HR 9105)
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Andromeda |
HD 225218 A | |
Right ascension | 00h 04m 36.58441s[1] |
Declination | +42° 05′ 33.0865″[1] |
Apparent magnitude (V) | 6.16[2] |
HD 225218 B | |
Right ascension | 00h 04m 36.67195s[3] |
Declination | +42° 05′ 27.8497″[3] |
Apparent magnitude (V) | 9.65[2] |
Characteristics | |
Spectral type | B9III[4] + F0V: |
U−B color index | 0.14 |
B−V color index | 0.15 |
Astrometry | |
HD 225218 A | |
Radial velocity (Rv) | −8.0[5] km/s |
Proper motion (μ) | RA: −10.367±0.266[1] mas/yr Dec.: −14.491±0.222[1] mas/yr |
Parallax (π) | 3.0041 ± 0.3539 mas[1] |
Distance | approx. 1,100 ly (approx. 330 pc) |
HD 225218 B | |
Proper motion (μ) | RA: −12.314±0.015[3] mas/yr Dec.: −16.129±0.015[3] mas/yr |
Parallax (π) | 4.4324 ± 0.0208 mas[3] |
Distance | 736 ± 3 ly (226 ± 1 pc) |
Orbit[6] | |
Period (P) | 70.12 yr |
Semi-major axis (a) | 0.165″ |
Eccentricity (e) | 0.515 |
Details | |
Luminosity | 394[7] L☉ |
Temperature | 7,611[7] K |
Rotation | 25[8] |
Other designations | |
Database references | |
SIMBAD | data |
Database references | |
SIMBAD | data |
HD 225218 is a quadruple star system in the northern constellation of Andromeda. The primary component, HD 225218 A, is a giant star with a stellar classification of B9III,[4] an apparent magnitude of 6.16,[2] and is a candidate Lambda Boötis star.[9] It has a fainter, magnitude 9.65 companion, HD 225218 B, at an angular separation of 5.2″ along a position angle of 171°.[2] The primary itself has been identified as a binary star system through interferometry, with the two components separated by 0.165″. The pair, HD 225218 Aa and Ab, orbit each other with a period of about 70 years and an eccentricity of 0.515.[6] Component B is likewise a spectroscopic binary.[9]
References
[edit]- ^ a b c d e Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
- ^ a b c d Mason, Brian D.; et al. (December 2001), "The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog", The Astronomical Journal, 122 (6): 3466–3471, Bibcode:2001AJ....122.3466M, doi:10.1086/323920
- ^ a b c d e Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
- ^ a b Cowley, A.; et al. (April 1969), "A study of the bright A stars. I. A catalogue of spectral classifications", Astronomical Journal, 74: 375–406, Bibcode:1969AJ.....74..375C, doi:10.1086/110819
- ^ Wilson, R. E. (1953), "General Catalogue of Stellar Radial Velocities", Carnegie Institute Washington D.C. Publication, Carnegie Institute of Washington, D.C., Bibcode:1953GCRV..C......0W
- ^ a b Malkov, O. Yu.; et al. (2012), "Dynamical Masses of a Selected Sample of Orbital Binaries", Astronomy & Astrophysics, 546: 5, Bibcode:2012A&A...546A..69M, doi:10.1051/0004-6361/201219774, A69
- ^ a b McDonald, I.; et al. (2012), "Fundamental Parameters and Infrared Excesses of Hipparcos Stars", Monthly Notices of the Royal Astronomical Society, 427 (1): 343–57, arXiv:1208.2037, Bibcode:2012MNRAS.427..343M, doi:10.1111/j.1365-2966.2012.21873.x, S2CID 118665352
- ^ Abt, Helmut A.; et al. (July 2002), "Rotational Velocities of B Stars", The Astrophysical Journal, 573 (1): 359–365, Bibcode:2002ApJ...573..359A, doi:10.1086/340590
- ^ a b Faraggiana, Rosanna; Bonifacio, Piercarlo (September 1999), "How many lambda Bootis stars are binaries?", Astronomy and Astrophysics, 349: 521–531, arXiv:astro-ph/9906009, Bibcode:1999A&A...349..521F