V Crucis
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Crux |
| Right ascension | 12h 56m 35.559s[1] |
| Declination | −57° 53′ 57.02″[1] |
| Apparent magnitude (V) | 8.74 - 11.13[2] |
| Characteristics | |
| Spectral type | Ce(Ne)[3] |
| Variable type | Mira[3] |
| Astrometry | |
| Radial velocity (Rv) | −19.90[4] km/s |
| Proper motion (μ) | RA: 0.507[1] mas/yr Dec.: 1.989[1] mas/yr |
| Parallax (π) | 0.7451 ± 0.0475 mas[1] |
| Distance | 4,400 ± 300 ly (1,340 ± 90 pc) |
| Absolute magnitude (MV) | -4.67[5] |
| Details | |
| Radius | 130[1] R☉ |
| Luminosity | 7,244[6] L☉ |
| Temperature | 3,075[6] K |
| Other designations | |
| Database references | |
| SIMBAD | data |
V Crucis is a carbon star in the constellation Crux. A Mira variable, its apparent magnitude ranges from 8.7 to 11.1 over 376.5 days.[3]
References
- ^ a b c d e f 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.
- ^ Pojmanski, G. (2002). "The All Sky Automated Survey. Catalog of Variable Stars. I. 0 h - 6 hQuarter of the Southern Hemisphere". Acta Astronomica. 52: 397–427. arXiv:astro-ph/0210283. Bibcode:2002AcA....52..397P.
- ^ a b c "V Crucis". AAVSO Website. American Association of Variable Star Observers. 4 January 2010. Retrieved 2019-12-11.
- ^ Gontcharov, G. A. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters. 32 (11): 759–771. arXiv:1606.08053. Bibcode:2006AstL...32..759G. doi:10.1134/S1063773706110065.
- ^ Guandalini, R.; Cristallo, S. (2013). "Luminosities of carbon-rich asymptotic giant branch stars in the Milky Way". Astronomy and Astrophysics. 555: A120. arXiv:1305.4203. Bibcode:2013A&A...555A.120G. doi:10.1051/0004-6361/201321225.
- ^ a b Bergeat, J.; Knapik, A.; Rutily, B. (2002). "Carbon-rich giants in the HR diagram and their luminosity function". Astronomy and Astrophysics. 390 (3): 967–986. Bibcode:2002A&A...390..967B. doi:10.1051/0004-6361:20020525.
- ^ "V Cru". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-12-11.
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