Astronomy:HD 34557
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Short description: Double star in the constellation Auriga
Observation data Equinox J2000.0]] (ICRS) | |
---|---|
Constellation | Auriga |
Right ascension | 05h 20m 14.66904s[1] |
Declination | +41° 05′ 10.3522″[1] |
Apparent magnitude (V) | 5.52[2] (5.58 + 8.55)[3] |
Characteristics | |
Spectral type | A3V[4] |
U−B color index | +0.04[2] |
B−V color index | +0.11[2] |
Astrometry | |
Radial velocity (Rv) | 22±4.2[5] km/s |
Proper motion (μ) | RA: −18.97[1] mas/yr Dec.: −53.43[1] mas/yr |
Parallax (π) | 11.77 ± 0.58[1] mas |
Distance | 280 ± 10 ly (85 ± 4 pc) |
Details | |
Radius | 1.6[6] R☉ |
Rotational velocity (v sin i) | 217[7] km/s |
Other designations | |
Database references | |
SIMBAD | data |
HD 34557 is a double star in the northern constellation of Auriga. The fainter star has an angular separation of 0.380″ from the primary component.[3] They have a combined apparent magnitude of 5.52,[2] making HD 34557 faintly visible to the naked eye from dark skies. Based upon parallax measurements made with the Hipparcos satellite, this system is roughly 280 light years away.[1] The primary component is spinning rapidly, with a projected rotational velocity of 217 km/s.[7] It has a stellar classification of A3V,[4] making it an A-type main sequence star.
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics 474 (2): 653–664, doi:10.1051/0004-6361:20078357, Bibcode: 2007A&A...474..653V
- ↑ 2.0 2.1 2.2 2.3 Deutschman, W. A.; Davis, R. J.; Schild, R. E. (February 1976), "The galactic distribution of interstellar absorption as determined from the Celescope catalog of ultraviolet stellar observations and a new catalog of UBV, H-beta photoelectric observations", Astrophysical Journal Supplement Series 30: 97–225, doi:10.1086/190359, Bibcode: 1976ApJS...30...97D
- ↑ 3.0 3.1 Eggleton, P. P. et al. (2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society 389 (2): 869–879, doi:10.1111/j.1365-2966.2008.13596.x, Bibcode: 2008MNRAS.389..869E
- ↑ 4.0 4.1 Cowley, A. et al. (April 1969), "A study of the bright A stars. I. A catalogue of spectral classifications", Astronomical Journal 74: 375–406, doi:10.1086/110819, Bibcode: 1969AJ.....74..375C
- ↑ Gontcharov, G. A. (November 2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters 32 (11): 759–771. doi:10.1134/S1063773706110065. Bibcode: 2006AstL...32..759G.
- ↑ Pasinetti Fracassini, L. E. et al. (2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition - Comments and statistics", Astronomy & Astrophysics 367 (2): 521–24, doi:10.1051/0004-6361:20000451, Bibcode: 2001A&A...367..521P
- ↑ 7.0 7.1 Royer, F. et al. (February 2007), "Rotational velocities of A-type stars. III. Velocity distributions", Astronomy and Astrophysics 463 (2): 671–682, doi:10.1051/0004-6361:20065224, Bibcode: 2007A&A...463..671R
References
Original source: https://en.wikipedia.org/wiki/HD 34557.
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