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HD 225218

From Wikipedia, the free encyclopedia
Quadruple star system in the constellation of Andromeda
HD 225218
Observation data
Epoch J2000.0      Equinox J2000.0
ConstellationAndromeda
HD 225218 A
Right ascension00h 04m 36.58441s[1]
Declination+42° 05′ 33.0865″[1]
Apparent magnitude (V)6.16[2]
HD 225218 B
Right ascension00h 04m 36.67195s[3]
Declination+42° 05′ 27.8497″[3]
Apparent magnitude (V)9.65[2]
Characteristics
Spectral typeB9III[4] + F0V:
U−Bcolor index0.14
B−Vcolor index0.15
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]
Distanceapprox. 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]
Distance736 ± 3 ly
(226 ± 1 pc)
Orbit[6]
Period (P)70.12yr
Semi-major axis (a)0.165″
Eccentricity (e)0.515
Details
Luminosity394[7] L
Temperature7,611[7] K
Rotation25[8]
Other designations
BD+41 4933,HD 225218,HIP 365,HR 9105,NSV 15012,SAO 36037,WDS J00046+4206.
Database references
SIMBADdata
Database references
SIMBADdata

HD 225218 is a quadruple star system in the northernconstellation ofAndromeda. The primary component, HD 225218 A, is agiant star with astellar classification of B9III,[4] anapparent magnitude of 6.16,[2] and is a candidateLambda Boötis star.[9] It has a fainter, magnitude 9.65 companion, HD 225218 B, at anangular separation of 5.2″ along aposition angle of 171°.[2] The primary itself has been identified as abinary star system throughinterferometry, 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 aneccentricity of 0.515.[6] Component B is likewise aspectroscopic binary.[9]

References

[edit]
  1. ^abcdeBrown, 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 atVizieR.
  2. ^abcdMason, 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
  3. ^abcdeBrown, 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 atVizieR.
  4. ^abCowley, 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
  5. ^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
  6. ^abMalkov, 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
  7. ^abMcDonald, 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
  8. ^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
  9. ^abFaraggiana, 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

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