Psi9 Aurigae (ψ9 Aur, ψ9 Aurigae) is the Bayer designation for a star in the northern constellation of Auriga. It is dimly visible to the naked eye with an apparent visual magnitude of 5.75.[2] Based upon an annual parallax shift of 2.59 mas,[1] the distance to this star is approximately 1,300 light-years (400 parsecs).
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Auriga |
Right ascension | 06h 56m 32.05791s[1] |
Declination | +46° 16′ 26.3867″[1] |
Apparent magnitude (V) | 5.75[2] |
Characteristics | |
Spectral type | B8 IIIe[3] |
U−B color index | –0.46[4] |
B−V color index | –0.06[4] |
Astrometry | |
Radial velocity (Rv) | –41.1[5] km/s |
Proper motion (μ) | RA: –2.93[1] mas/yr Dec.: +4.07[1] mas/yr |
Parallax (π) | 2.59 ± 0.38 mas[1] |
Distance | approx. 1,300 ly (approx. 390 pc) |
Details | |
Radius | 3.7[2] R☉ |
Rotational velocity (v sin i) | 235[6] km/s |
Other designations | |
The spectrum of Psi9 Aurigae matches a giant star with a stellar classification of B8 IIIe.[3] The 'e' suffix indicates this is a Be star that shows emission lines of hydrogen in its spectrum. This is caused by a circumstellar shell of hot gas. The emission undergoes variability on a time scale of sixteen years.[3]
References
- ^ a b c d e f van Leeuwen, Floor (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752v1, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357.
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ignored (help) Note: see VizieR catalogue I/311. - ^ a b c Pasinetti Fracassini, L. E.; et al. (2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition - Comments and statistics", Astronomy and Astrophysics, 367: 521–524, arXiv:astro-ph/0012289, Bibcode:2001A&A...367..521P, doi:10.1051/0004-6361:20000451.
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ignored (help) - ^ a b c Ghosh, K. K. (1989), "Search for rapid spectral variability in Psi(9) Aurigae", Publications of the Astronomical Society of the Pacific, 101: 839–843, Bibcode:1989PASP..101..839G, doi:10.1086/132504.
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ignored (help) - ^ a b Crawford, D. L. (1963), "U, b, v, and Hβ Photometry for the Bright B8- and B9-TYPE Stars", Astrophysical Journal, 137: 530, Bibcode:1963ApJ...137..530C, doi:10.1086/147526.
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ignored (help) - ^ Wilson, Ralph Elmer (1953), General Catalogue of Stellar Radial Velocities, Washington: Carnegie Institution of Washington, Bibcode:1953QB901.W495......
- ^ Abt, Helmut A.; Levato, Hugo; Grosso, Monica (2002), "Rotational Velocities of B Stars", The Astrophysical Journal, 573 (1): 359–365, Bibcode:2002ApJ...573..359A, doi:10.1086/340590.
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ignored (help) - ^ "HR 2568 -- Be Star", SIMBAD Astronomical Database, Centre de Données astronomiques de Strasbourg, retrieved 2012-08-23.