V1401 Aquilae
Appearance
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Aquila |
Right ascension | 20h 05m 05.41390s |
Declination | −11° 35′ 57.8808″ |
Apparent magnitude (V) | 6.39 |
Characteristics | |
Spectral type | F1III |
B−V color index | 0.52 |
Variable type | SRd[1] |
Astrometry | |
Radial velocity (Rv) | -12.1 ± 2 km/s |
Proper motion (μ) | RA: -2.19 ± 0.44 mas/yr Dec.: -14.18 ± 0.43 mas/yr |
Parallax (π) | 2.56 ± 0.97 mas |
Distance | approx. 1,300 ly (approx. 400 pc) |
Other designations | |
Database references | |
SIMBAD | data |
V1401 Aquilae is semi-regular pulsating star in the constellation Aquila. Its evolutionary status is unclear, and it has been classified as a post-AGB object, a UU Herculis variable or belonging to the W Virginis variable subclass of the type II Cepheids. It has a low metallicity.[2] V1401 Aquilae was a latter designation of 64 Sagittarii.[3]
References
- ^ Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/gcvs. Originally published in: 2009yCat....102025S. 1. Bibcode:2009yCat....102025S.
- ^ Reyniers, M.; Cuypers, J. (2005). "The evolutionary status of the bright high-latitude supergiant HD 190390". Astronomy and Astrophysics. 432 (2): 595–608. arXiv:astro-ph/0411493. Bibcode:2005A&A...432..595R. doi:10.1051/0004-6361:20042097.
- ^ Wagman, M. (August 1987). "Flamsteed's Missing Stars". Journal for the History of Astronomy. 18 (3): 209, 221. Bibcode:1987JHA....18..209W. doi:10.1177/002182868701800305.