HD 36041 is giant star in the northern constellation Auriga. It has an apparent magnitude of 6.37,[2] making it faintly visible to the naked eye.
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Auriga |
Right ascension | 05h 30m 45.08329s[1] |
Declination | +39° 49′ 33.2897″[1] |
Apparent magnitude (V) | 6.37[2] |
Characteristics | |
Spectral type | G9III[3] |
U−B color index | +0.76[2] |
B−V color index | +0.97[2] |
Astrometry | |
Radial velocity (Rv) | +11.5[4] km/s |
Proper motion (μ) | RA: +21.73[1] mas/yr Dec.: -36.69[1] mas/yr |
Parallax (π) | 5.70 ± 0.48 mas[1] |
Distance | 570 ± 50 ly (180 ± 10 pc) |
Details | |
Luminosity | 86.2[5] L☉ |
Temperature | 5,042[5] K |
Other designations | |
Database references | |
SIMBAD | data |
References
edit- ^ a b c d e van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357, S2CID 18759600
- ^ a b c d Lutz, T. E.; Lutz, J. H. (June 1977), "Spectral classification and UBV photometry of bright visual double stars", Astronomical Journal, 82: 431–434, Bibcode:1977AJ.....82..431L, doi:10.1086/112066
- ^ Halliday, Ian (September 1955), "Luminosity Function and Space Motions of G8-K1 Stars Derived from Spectroscopic Parallaxes", Astrophysical Journal, 122: 222, Bibcode:1955ApJ...122..222H, doi:10.1086/146080
- ^ 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
- ^ a b McDonald, I.; Zijlstra, A. A; Boyer, M. L. (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.
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