HD 125351
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Boötes |
Right ascension | 14h 17m 59.81955s[1] |
Declination | +35° 30′ 34.2208″[1] |
Apparent magnitude (V) | ±0.0007 4.9660[2] |
Characteristics | |
Spectral type | K1III[3] |
Astrometry | |
Radial velocity (Rv) | ±0.3 −21.6[2] km/s |
Proper motion (μ) | RA: 4.87[1] mas/yr Dec.: 14.40[1] mas/yr |
Parallax (π) | 13.97 ± 0.39[1] mas |
Distance | 233 ± 7 ly (72 ± 2 pc) |
Details | |
Surface gravity (log g) | 2.25[4] cgs |
Temperature | 4,650[4] K |
Metallicity [Fe/H] | −0.03[4] dex |
Other designations | |
HD 125351 or A Boötis (A Boo) is spectroscopic binary[5] in the constellation Boötes. The system has an apparent magnitude of +4.97, with a spectrum matching a K-type giant star. It is approximately 233 light years from Earth.
References
- 1 2 3 4 5 van Leeuwen, F. (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 Famaey, B.; et al. (2005), "Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters", Astronomy and Astrophysics 430: 165–186, Bibcode:2005A&A...430..165F, doi:10.1051/0004-6361:20041272.
- ↑ Griffin, R. F. (1961), "Photoelectric measurements of the lambda5250A Fe I triplet and the D lines in G and K stars", Monthly Notices of the Royal Astronomical Society 122: 181, Bibcode:1961MNRAS.122..181G, doi:10.1093/mnras/122.3.181.
- 1 2 3 Luck, R. Earle; Challener, Sharon L. (December 1995), "Chemical Abundances for Very Strong-Lined Giants", Astronomical Journal 110: 2968, Bibcode:1995AJ....110.2968L, doi:10.1086/117741.
- ↑ Pourbaix, D.; Boffin, H. M. J. (February 2003), "Reprocessing the Hipparcos Intermediate Astrometric Data of spectroscopic binaries. II. Systems with a giant component", Astronomy and Astrophysics 398: 1163–1177, arXiv:astro-ph/0211483, Bibcode:2003A&A...398.1163P, doi:10.1051/0004-6361:20021736.
External links
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