HD 191104
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Aquila |
| Right ascension | 20h 07m 50.36773s[1] |
| Declination | +09° 23′ 59.4022″[1] |
| Apparent magnitude (V) | 6.443[2] |
| Characteristics | |
| Spectral type | F3V[3] |
| U−B color index | -0.033[2] |
| B−V color index | +0.472[2] |
| Astrometry | |
| Radial velocity (Rv) | −27[4] km/s |
| Proper motion (μ) | RA: +46.75[1] mas/yr Dec.: +28.81[1] mas/yr |
| Parallax (π) | 25.40 ± 1.00[1] mas |
| Distance | 128 ± 5 ly (39 ± 2 pc) |
| Other designations | |
| Database references | |
| SIMBAD | data |
HD 191104 is a triple star system in the equatorial constellation of Aquila. Two of the components form a close spectroscopic binary system, while a third stars orbits the pair at a greater distance.[5]
References
- 1 2 3 4 5 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 - 1 2 3 Rakos, K. D.; et al. (February 1982), "Photometric and astrometric observations of close visual binaries", Astronomy and Astrophysics Supplement Series, 47: 221–235, Bibcode:1982A&AS...47..221R
- ↑ Abt, H. A. (March 1981), "Visual multiples. VII - MK classifications", Astrophysical Journal Supplement Series, 45: 437−456, Bibcode:1981ApJS...45..437A, doi:10.1086/190719
- ↑ Wilson, R. E. (1953), General Catalogue of Stellar Radial Velocities, Carnegie Institute of Washington, D.C., Bibcode:1953GCRV..C......0W
- ↑ Tokovinin, Andrei (April 2014), "From Binaries to Multiples. II. Hierarchical Multiplicity of F and G Dwarfs", The Astronomical Journal, 147 (4): 14, arXiv:1401.6827, Bibcode:2014AJ....147...87T, doi:10.1088/0004-6256/147/4/87, 87
External links
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