R Crucis
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Crux |
Right ascension | 12h 23m 37.68840s[2] |
Declination | −61° 37′ 44.8570″[2] |
Apparent magnitude (V) | 6.89[3] |
Characteristics | |
Spectral type | F6-G2Ib-II[4] or F7Ib/II[5] |
B−V color index | 0.67±0.02[3] |
Variable type | δ Cep[6]
|
Details | |
dex | |
Database references | |
SIMBAD | data |
R Crucis is a
light years from the Sun based on parallax,[7] but it is drifting closer with a radial velocity of −13.5 km/s.[3]
This is a Classical Cepheid, or
radius of the Sun (44.6 R☉), but the radius varies by 5 R☉ during each pulsation.[11] It has a near solar metallicity and the atmospheric abundances indicate it is likely past first dredge-up.[9]
A candidate companion star has been detected at an
projected separation of 6,330 AU. The Hubble WFC3 shows a closer companion at a separation of 1.9″.[12] The system is a source for X-ray emission but the contributing component is unclear.[13]
References
- Bibcode:1977MmRAS..83...69D. Retrieved 18 December 2021.
- ^ .
- ^ S2CID 119257644.
- ^ a b Watson, Christopher (4 January 2010). "R Crucis". AAVSO Website. American Association of Variable Star Observers. Retrieved 12 March 2014.
- Bibcode:1978mcts.book.....H.
- ^ S2CID 125853869.
- ^ S2CID 18759600.
- Bibcode:2005AcA....55..247M.
- ^ S2CID 122521758.
- ^ "R Cru". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-02-14.
- Bibcode:2005AcA....55..247M.
- S2CID 119248298. 129.
- S2CID 118928066. 67.