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HD 29573

From Wikipedia, the free encyclopedia
Binary star system in the constellation Eridanus
HD 29573
Observation data
Epoch J2000      Equinox J2000
ConstellationEridanus
Right ascension04h 38m 53.55015s[1]
Declination−12° 07′ 23.0681″[1]
Apparent magnitude (V)4.99[2](5.19 + 7.22)[3]
Characteristics
Spectral typeA0 V(A1 + F2)[2]
B−Vcolor index0.074±0.003[4]
Astrometry
Radial velocity (Rv)+2.9±0.8[5] km/s
Proper motion (μ)RA: −60.614[1]mas/yr
Dec.: −16.417[1]mas/yr
Parallax (π)14.2348±0.3656 mas[1]
Distance229 ± 6 ly
(70 ± 2 pc)
Absolute magnitude (MV)0.73[4]
Orbit[2]
Period (P)40.9±1.386yr
Semi-major axis (a)0.2844±0.0055
Eccentricity (e)0.759±0.180
Inclination (i)75.5±2.2°
Longitude of the node (Ω)152.0±1.8°
Periastronepoch (T)2003.805
Argument of periastron (ω)
(secondary)
284.1±11.0°
Details
HD 29573 A
Mass2.28[2] M
Luminosity51.8+4.6
−4.3
[6] L
Temperature8,892+103
−102
[6] K
Rotational velocity (v sin i)27[6] km/s
HD 29573 B
Mass1.56[2] M
Other designations
BD−12°955,GJ 9161,HD 29573,HIP 21644,HR 1483,SAO 149789,WDS J04389-1207AB[7]
Database references
SIMBADdata

HD 29573 is abinary star[3] system in theconstellationEridanus. It has a combinedapparent visual magnitude of 4.99,[2] making it visible to the naked eye. Based upon an annualparallax shift of14.23 mas,[1] it is located 229 light years from theSun. The system is moving further away from Earth with a heliocentricradial velocity of +3 km/s.[5]

The binary nature of this system was discovered through observations made with theHipparcos spacecraft. The pairorbit each other with aperiod of 41 years and aneccentricity of 0.8.[2] The magnitude 5.19[3] primary component has a class of A1,[2] 2.28[2] times themass of the Sun, and is a suspectedchemically peculiar star.[8] The secondary has magnitude 7.22,[3] 1.56[2] times the Sun's mass, and a class of F2.[2] The system has a possibleinfrared excess[9] due to circumstellar dust.[10]

References

[edit]
  1. ^abcdefVallenari, A.; et al. (Gaia collaboration) (2023)."Gaia Data Release 3. Summary of the content and survey properties".Astronomy and Astrophysics.674: A1.arXiv:2208.00211.Bibcode:2023A&A...674A...1G.doi:10.1051/0004-6361/202243940.S2CID 244398875. Gaia DR3 record for this source atVizieR.
  2. ^abcdefghijkCvetković, Z.; et al. (March 2014), "Orbits for Eight Hipparcos Double Stars",The Astronomical Journal,147 (3): 9,Bibcode:2014AJ....147...62C,doi:10.1088/0004-6256/147/3/62,S2CID 121138730, 62.
  3. ^abcdEggleton, P. P.; Tokovinin, A. A. (2008), "A catalogue of multiplicity among bright stellar systems",Monthly Notices of the Royal Astronomical Society,389 (2): 869,arXiv:0806.2878,Bibcode:2008MNRAS.389..869E,doi:10.1111/j.1365-2966.2008.13596.x,S2CID 14878976.
  4. ^abAnderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation",Astronomy Letters,38 (5): 331,arXiv:1108.4971,Bibcode:2012AstL...38..331A,doi:10.1134/S1063773712050015,S2CID 119257644.
  5. ^abde Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project",Astronomy & Astrophysics,546: 14,arXiv:1208.3048,Bibcode:2012A&A...546A..61D,doi:10.1051/0004-6361/201219219,S2CID 59451347, A61.
  6. ^abcZorec, J.; Royer, F. (2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities",Astronomy & Astrophysics,537: A120,arXiv:1201.2052,Bibcode:2012A&A...537A.120Z,doi:10.1051/0004-6361/201117691,S2CID 55586789.
  7. ^"HD 29573".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2018-07-23.
  8. ^Renson, P.; Manfroid, J. (May 2009), "Catalogue of Ap, HgMn and Am stars",Astronomy and Astrophysics,498 (3):961–966,Bibcode:2009A&A...498..961R,doi:10.1051/0004-6361/200810788.
  9. ^Shylaja, B. S.; Ashok, N. M. (June 2002), "IR observations of Am stars",Bulletin of the Astronomical Society of India,30:491–500,Bibcode:2002BASI...30..491S.
  10. ^Kamp, I.; et al. (June 2002), "Do dusty A stars exhibit accretion signatures in their photospheres?",Astronomy and Astrophysics,388 (3):978–984,arXiv:astro-ph/0204449,Bibcode:2002A&A...388..978K,doi:10.1051/0004-6361:20020493,S2CID 18191361.
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