From Wikipedia, the free encyclopedia
60 Andromedae
Location of 60 Andromedae (circled)
Observation data
Epoch J2000       Equinox J2000
Constellation Andromeda
Right ascension 02h 13m 13.32387s [1]
Declination +44° 13′ 53.9546″ [1]
Apparent magnitude (V) +4.82 [2]
Characteristics
Spectral type K3.5 III Ba0.4 [3]
U−B color index +1.74 [2]
B−V color index +1.48 [2]
Astrometry
Radial velocity (Rv)–46.3 [4] km/s
Proper motion (μ) RA: –20.90 [1]  mas/ yr
Dec.: –14.46 [1]  mas/ yr
Parallax (π)6.15 ± 0.63  mas [1]
Distanceapprox. 530  ly
(approx. 160  pc)
Orbit [5]
Period (P)748.2±0.4 days
Semi-major axis (a)2.4±0.6 mas
Eccentricity (e)0.80
Inclination (i)54.1±19.9°
Longitude of the node (Ω)344.5±10.3°
Periastron epoch (T)37886±11 HJD
Argument of periastron (ω)
(secondary)
358±6°
Semi-amplitude (K1)
(primary)
4.88 km/s
Details
60 And A
Mass2.0+0.7
−0.3
[6]  M
Surface gravity (log g)1.70±0.44 [7]  cgs
Temperature4054±42 [7]  K
Metallicity [Fe/H]−0.13±0.12 [7]  dex
60 And B
Mass0.5±0.1 [6]  M
Other designations
b Andromedae, [8] BD+43 447, HD 13520, HIP 10340, HR 643, IRAS 02100+4359, SAO 37867, PPM 44882
Database references
SIMBAD data

60 Andromedae (abbreviated 60 And) is a star system in the northern constellation of Andromeda, located to the west-northwest of Gamma Andromedae. 60 Andromedae is the Flamsteed designation though the star also bears the Bayer designation b Andromedae. It is bright enough to be seen by the naked eye with an apparent visual magnitude of 4.82. [2] Based upon parallax measurements made during the Hipparcos mission, it is at a distance of roughly 530 light-years (160 parsecs) from Earth. [1]

This system is known to have three components. The primary is a giant star with a stellar classification of K3.5 III Ba0.4, meaning that an overabundance of barium ionized one time is observed in the spectrum of the star, making it a barium star. The secondary component is likely a white dwarf with a period of 748.2 days and an eccentricity of 0.34. There is a third component at an angular separation of 0.22  arcseconds. [3]

References

  1. ^ a b c d e f 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, S2CID  18759600.
  2. ^ a b c d Argue, A. N. (1966), "UBV photometry of 550 F, G and K type stars", Monthly Notices of the Royal Astronomical Society, 133 (4): 475–493, Bibcode: 1966MNRAS.133..475A, doi: 10.1093/mnras/133.4.475.
  3. ^ a b 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, S2CID  14878976.
  4. ^ Wilson, Ralph Elmer (1953), "General Catalogue of Stellar Radial Velocities", Carnegie Institute Washington D.C. Publication, Washington: Carnegie Institution of Washington, Bibcode: 1953GCRV..C......0W.
  5. ^ Ren, Shulin; Fu, Yanning (March 2013), "Hipparcos Photocentric Orbits of 72 Single-lined Spectroscopic Binaries", The Astronomical Journal, 145 (3): 7, Bibcode: 2013AJ....145...81R, doi: 10.1088/0004-6256/145/3/81, S2CID  120199240, 81.
  6. ^ a b 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 (3): 1163–1177, arXiv: astro-ph/0211483, Bibcode: 2003A&A...398.1163P, doi: 10.1051/0004-6361:20021736, S2CID  12361870.
  7. ^ a b c Koleva, M.; Vazdekis, A. (February 2012), "Stellar population models in the UV. I. Characterisation of the New Generation Stellar Library", Astronomy & Astrophysics, 538: A143, arXiv: 1111.5449, Bibcode: 2012A&A...538A.143K, doi: 10.1051/0004-6361/201118065, S2CID  53999614.
  8. ^ Tirion; Rappaport; Lovi (1987). Willmann-Bell, Inc. (ed.). Uranometria 2000.0 - Volume II - The Southern Hemisphere to +6°. Richmond, Virginia, USA. ISBN  0-943396-15-8.

External links

  1. "* 60 And". SIMBAD. Centre de données astronomiques de Strasbourg.