HD 41162
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Auriga |
| Right ascension | 06h 05m 02.58110s[1] |
| Declination | +37° 57′ 51.3817″[1] |
| Apparent magnitude (V) | 6.32[2] |
| Characteristics | |
| Spectral type | G8III + F0V:[3] |
| Astrometry | |
| Radial velocity (Rv) | −1.1±0.3[4] km/s |
| Proper motion (μ) | RA: -4.06[1] mas/yr Dec.: -6.25[1] mas/yr |
| Parallax (π) | 5.47 ± 0.89[1] mas |
| Distance | approx. 600 ly (approx. 180 pc) |
| Other designations | |
| Database references | |
| SIMBAD | data |
HD 41162 is a star in a double system.
References
- 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
- Oja, T. (August 1991), "UBV photometry of stars whose positions are accurately known. VI", Astronomy and Astrophysics Supplement Series, 89 (2): 415–419, Bibcode:1991A&AS...89..415O
- Abt, Helmut A. (May 2008), "Visual Multiples. IX. MK Spectral Types", The Astrophysical Journal Supplement Series, 176 (1): 216–217, Bibcode:2008ApJS..176..216A, doi:10.1086/525529
- Famaey, B.; et al. (2005). "Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters". Astronomy and Astrophysics. 430: 165–186. arXiv:astro-ph/0409579. Bibcode:2005A&A...430..165F. doi:10.1051/0004-6361:20041272.
External links
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