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HD 29573

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Binary star system in the constellation Eridanus
HD 29573
Observation data
Epoch J2000      Equinox J2000
Constellation Eridanus
Right ascension 04 38 53.55015
Declination −12° 07′ 23.0681″
Apparent magnitude (V) 4.99 (5.19 + 7.22)
Characteristics
Spectral type A0 V (A1 + F2)
B−V color index 0.074±0.003
Astrometry
Radial velocity (Rv)+2.9±0.8 km/s
Proper motion (μ) RA: −60.614 mas/yr
Dec.: −16.417 mas/yr
Parallax (π)14.2348 ± 0.3656 mas
Distance229 ± 6 ly
(70 ± 2 pc)
Absolute magnitude (MV)0.73
Orbit
Period (P)40.9±1.386 yr
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°
Periastron epoch (T)2003.805
Argument of periastron (ω)
(secondary)
284.1±11.0°
Details
HD 29573 A
Mass2.28 M
Luminosity51.8+4.6
−4.3 L
Temperature8,892+103
−102 K
Rotational velocity (v sin i)27 km/s
HD 29573 B
Mass1.56 M
Other designations
BD−12° 955, GJ 9161, HD 29573, HIP 21644, HR 1483, SAO 149789, WDS J04389-1207AB
Database references
SIMBADdata

HD 29573 is a binary star system in the constellation Eridanus. It has a combined apparent visual magnitude of 4.99, making it visible to the naked eye. Based upon an annual parallax shift of 14.23 mas, it is located 229 light years from the Sun. The system is moving further away from Earth with a heliocentric radial velocity of +3 km/s.

The binary nature of this system was discovered through observations made with the Hipparcos spacecraft. The pair orbit each other with a period of 41 years and an eccentricity of 0.8. The magnitude 5.19 primary component has a class of A1, 2.28 times the mass of the Sun, and is a suspected chemically peculiar star. The secondary has magnitude 7.22, 1.56 times the Sun's mass, and a class of F2. The system has a possible infrared excess due to circumstellar dust.

References

  1. ^ Vallenari, 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 at VizieR.
  2. ^ Cvetković, 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. ^ Eggleton, 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. ^ Anderson, 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. ^ de 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. ^ Zorec, 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. Retrieved 2018-07-23.
  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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