| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Auriga |
| Right ascension | 05h 39m 18.3132s[2] |
| Declination | +29° 12′ 54.788″[2] |
| Apparent magnitude (V) | 6.02–6.06[3] |
| Characteristics | |
| Spectral type | B2IV-V[4] |
| U−B color index | −0.5 |
| B−V color index | +0.16 |
| Variable type | SPB |
| Astrometry | |
| Radial velocity (Rv) | 22.90 ± 1.9[5] km/s |
| Proper motion (μ) | RA: −0.82[6] mas/yr Dec.: −7.11[6] mas/yr |
| Parallax (π) | 1.0114 ± 0.1708 mas[2] |
| Distance | approx. 3,200 ly (approx. 1,000 pc) |
| Details | |
| Luminosity | 322[7] L☉ |
| Temperature | 7400[7] K |
| Other designations | |
| Database references | |
| SIMBAD | data |
V433 Aurigae is a variable star in the constellation Auriga. It is a slowly pulsating B star (SPB) that ranges from apparent magnitude 6.02 to 6.06 over 4.6 days.[3] Using a Hipparcos-derived distance of about 1,060 light-years (324 pc), it shines with a luminosity approximately 322 times that of the Sun and has a surface temperature of 7400 K.[7] However, measurements by Gaia indicate a much higher distance of 3,200 light-years (980 pc).[2]
References
- ^ "Hipparcos Tools Interactive Data Access". Hipparcos. ESA. Retrieved 8 December 2021.
- ^ a b c d Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- ^ a b Watson, Christopher (4 January 2010). "V433 Aurigae". The International Variable Star Index. American Association of Variable Star Observers. Retrieved 4 August 2015.
- ^ a b "V433 Aur". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-03-21.
- ^ Gontcharov, G. A. (2006). "Pulkovo Compilation of Radial Velocities for 35495 Hipparcos stars in a common system". Astronomy Letters. 32 (11): 759–771. arXiv:1606.08053. Bibcode:2006AstL...32..759G. doi:10.1134/S1063773706110065. S2CID 119231169.
- ^ a b van Leeuwen, F.; et al. (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 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.
| Stars |
| ||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| |||||||||||||
| Star clusters |
| ||||||||||||
| Nebulae |
| ||||||||||||
| |||||||||||||
| |||||||||||||
 | This variable star–related article is a stub. You can help Wikipedia by expanding it. |
This page was last edited on 23 May 2023, at 06:24