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HD 151613

From Wikipedia, the free encyclopedia
Binary star system in the constellation in the constellation of Draco
HD 151613
Observation data
Epoch J2000      Equinox J2000
ConstellationDraco[1]
Right ascension16h 45m 17.88121s[2]
Declination+56° 46′ 54.7985″[2]
Apparent magnitude (V)4.84[1]
Characteristics
Spectral typeF2 V[3]
B−Vcolor index0.375±0.013[1]
Astrometry
Radial velocity (Rv)−2.0[4] km/s
Proper motion (μ)RA: 24.85mas/yr
Dec.: 67.07mas/yr
Parallax (π)39.2932±0.3182 mas[2]
Distance83.0 ± 0.7 ly
(25.4 ± 0.2 pc)
Absolute magnitude (MV)2.71[1]
Orbit[5]
Period (P)363.57 d
Eccentricity (e)0.35
Periastronepoch (T)2415232.4 JD
Argument of periastron (ω)
(secondary)
80.7°
Semi-amplitude (K1)
(primary)
6.0 km/s
Details
Mass1.43[4] M
Radius1.6[6] R
Luminosity6.91[1] L
Surface gravity (log g)4.05[4] cgs
Temperature6,630[7] K
Metallicity[Fe/H]−0.23[4] dex
Rotational velocity (v sin i)47.5±2.4[7] km/s
Age2.30[4] Gyr
Other designations
BD+57°1702,FK5 627,GJ 9578,HD 151613,HIP 82020,HR 6237,SAO 30076,WDS 16453+5647[8]
Database references
SIMBADdata

HD 151613 is abinary star[5] system in the northerncircumpolar constellation ofDraco. It is visible to the naked eye with anapparent visual magnitude of 4.84.[1] The distance to this star, as estimated from its annualparallax shift of39.3 mas,[2] is 83 light years. It is moving closer to the Earth with a heliocentricradial velocity of −2 km/s.[4]

This is a single-linedspectroscopic binary[3] system with anorbital period of 363.57 days and aneccentricity of 0.35.[5] The pair were resolved throughspeckle interferometry in 1977, showing anangular separation of0.041. They were later resolved in 1981 with a separation of0.047″, but were unresolved during 20 other attempts between 1976–1991.[9] The system is a source ofX-ray emission.[10] The visible component is anF-type main-sequence star with astellar classification of F2 V.[3] It is around 2.3 billion years old[4] with aprojected rotational velocity of 48 km/s.[7]

References

[edit]
  1. ^abcdefAnderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation",Astronomy Letters,38 (5): 331,arXiv:1108.4971,Bibcode:2012AstL...38..331A,doi:10.1134/S1063773712050015. XHIP record for this object atVizieR.
  2. ^abcdBrown, A. G. A.; et al. (Gaia collaboration) (August 2018)."Gaia Data Release 2: Summary of the contents and survey properties".Astronomy & Astrophysics.616. A1.arXiv:1804.09365.Bibcode:2018A&A...616A...1G.doi:10.1051/0004-6361/201833051.
  3. ^abcAbt, Helmut A. (2009), "MK Classifications of Spectroscopic Binaries",The Astrophysical Journal Supplement,180 (1):117–18,Bibcode:2009ApJS..180..117A,doi:10.1088/0067-0049/180/1/117,S2CID 122811461.
  4. ^abcdefgCasagrande, L.; et al. (June 2011), "New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s). Improved astrophysical parameters for the Geneva-Copenhagen Survey",Astronomy and Astrophysics,530: A138,arXiv:1103.4651,Bibcode:2011A&A...530A.138C,doi:10.1051/0004-6361/201016276,S2CID 56118016.
  5. ^abcPourbaix, D.; et al. (2004), "SB9: The Ninth Catalogue of Spectroscopic Binary Orbits",Astronomy & Astrophysics,424:727–732,arXiv:astro-ph/0406573,Bibcode:2004A&A...424..727P,doi:10.1051/0004-6361:20041213,S2CID 119387088.
  6. ^Pasinetti Fracassini, L. E.; Pastori, L.; Covino, S.; Pozzi, A. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition",Astronomy and Astrophysics,367 (2):521–524,arXiv:astro-ph/0012289,Bibcode:2001A&A...367..521P,doi:10.1051/0004-6361:20000451,S2CID 425754.
  7. ^abcReiners, Ansgar (January 2006), "Rotation- and temperature-dependence of stellar latitudinal differential rotation",Astronomy and Astrophysics,446 (1):267–277,arXiv:astro-ph/0509399,Bibcode:2006A&A...446..267R,doi:10.1051/0004-6361:20053911,S2CID 8642707
  8. ^"HD 151613".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2018-07-18.
  9. ^Hartkopf, William I.; Mason, Brian D. (September 2009), "Speckle Interferometry at Mount Wilson Observatory: Observations Obtained in 2006-2007 and 35 New Orbits",The Astronomical Journal,138 (3):813–826,Bibcode:2009AJ....138..813H,doi:10.1088/0004-6256/138/3/813.
  10. ^Haakonsen, Christian Bernt; Rutledge, Robert E. (September 2009), "XID II: Statistical Cross-Association of ROSAT Bright Source Catalog X-ray Sources with 2MASS Point Source Catalog Near-Infrared Sources",The Astrophysical Journal Supplement,184 (1):138–151,arXiv:0910.3229,Bibcode:2009ApJS..184..138H,doi:10.1088/0067-0049/184/1/138,S2CID 119267456.


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