107 Aquarii
From Wikipedia, the free encyclopedia
Observation data Epoch J2000.0 (ICRS) Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Aquarius |
Right ascension | 23h 46m 00.92254s[1] |
Declination | –18° 40′ 42.0313″[1] |
Apparent magnitude (V) | +5.305[2] (5.72/6.72)[3] |
Characteristics | |
Spectral type | F2 III + F2 V[3] |
U−B color index | +0.141[2] |
B−V color index | +0.287[2] |
Astrometry | |
Radial velocity (Rv) | –1.8[4] km/s |
Proper motion (μ) | RA: +130.33[1] mas/yr Dec.: +10.84[1] mas/yr |
Parallax (π) | 13.66 ± 1.05 mas |
Distance | 240 ± 20 ly (73 ± 6 pc) |
Details | |
Rotational velocity (v sin i) | 70[5] km/s |
Other designations | |
Data sources: | |
Hipparcos Catalogue, CCDM (2002), Bright Star Catalogue (5th rev. ed.) |
107 Aquarii ( i2 Aquarii) is the Flamsteed designation for a double star in the equatorial constellation of Aquarius. The pair have an angular separation of 6.787 arcseconds.[3] They have a combined apparent visual magnitude of +5.305,[2] with individual magnitudes of 5.72 and 6.72.[3] The annual parallax shift is 13.66 milliarcseconds with an 8% margin of error.[1] This indicates the system is at a distance of around 240 light-years (74 parsecs) from Earth.
References
- ↑ 1.0 1.1 1.2 1.3 1.4 van Leeuwen, F. (November 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.
- ↑ 2.0 2.1 2.2 2.3 Weiss, R. (February 1982), "Photometric and astrometric observations of close visual binaries", Astronomy and Astrophysics Supplement Series 47: 221–235, Bibcode:1982A&AS...47..221R
- ↑ 3.0 3.1 3.2 3.3 Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society 389 (2): 869–879, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x.
- ↑ Wilson, R. E. (1953), General Catalogue of Stellar Radial Velocities, Carnegie Institute of Washington D.C., Bibcode:1953GCRV..C......0W.
- ↑ Royer, F.; Zorec, J.; Gómez, A. E. (February 2007), "Rotational velocities of A-type stars. III. Velocity distributions", Astronomy and Astrophysics 463 (2): 671–682, arXiv:astro-ph/0610785, Bibcode:2007A&A...463..671R, doi:10.1051/0004-6361:20065224.
- ↑ "CCDM J23460-1841AB -- Double or multiple star", SIMBAD Astronomical Object Database, retrieved 2007-07-14
External links
|
This article is issued from Wikipedia. The text is available under the Creative Commons Attribution/Share Alike; additional terms may apply for the media files.