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Upsilon1 Centauri

From Wikipedia, the free encyclopedia
Star in the constellation Centaurus
For other stars with this Bayer designation, seeυ Centauri.
υ1 Centauri
Location of υ1 Centauri (circled in red)
Observation data
Epoch J2000.0      Equinox J2000.0
ConstellationCentaurus[1]
Right ascension13h 58m 40.75s[2]
Declination−44° 48′ 12.9″[2]
Apparent magnitude (V)+3.87[1]
Characteristics
Spectral typeB2 IV/V[3]
B−Vcolor index−0.208±0.011[1]
Astrometry
Radial velocity (Rv)+9.2±1.4[4] km/s
Proper motion (μ)RA: −27.51±0.15mas/yr[2]
Dec.: −22.44±0.13mas/yr[2]
Parallax (π)7.63±0.16 mas[2]
Distance427 ± 9 ly
(131 ± 3 pc)
Absolute magnitude (MV)−1.72[1]
Details
Mass7.9±0.1[5] M
Radius3.74±0.34[6] R
Luminosity1,884[1] L
Surface gravity (log g)4.15±0.07[6] cgs
Temperature21,411±377[6] K
Rotational velocity (v sin i)124[4] km/s
Age13.0±2.0[5] Myr
Other designations
υ1 Cen,CD−44°9010,FK5 3112,HD 121790,HIP 68282,HR 5249,SAO 224585[7]
Database references
SIMBADdata

Upsilon1 Centauri is a single[8]star in the southernconstellation ofCentaurus. Its name is aBayer designation that isLatinized from υ1 Centauri, and abbreviated Upsilon1 Cen or υ1 Cen. This star has a blue-white hue and is visible to thenaked eye with anapparent visual magnitude of +3.87.[1] The distance to this object is approximately 427 light years based onparallax,[2] and is receding with aradial velocity of +9 km/s.[4] It is a member of the Lower Centaurus Crux group of theScorpius–Centaurus association.[1]

Thestellar classification of this object is B2 IV/V,[1] matching a massiveB-type star with aluminosity class displaying mixed traits of amain sequence and asubgiant star. It is 13[5] million years old and is spinning with aprojected rotational velocity of 124 km/s.[4] The star has 7.9[5] times themass of the Sun and 3.7[6] times theSun's radius. It is radiating 1,884[1] times theluminosity of the Sun from itsphotosphere at aneffective temperature of 21,411 K.[6]

References

[edit]
  1. ^abcdefghiAnderson, 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. ^abcdevan 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,S2CID 18759600.Vizier catalog entry
  3. ^Hiltner, W. A.; et al. (July 1969), "MK Spectral Types for Bright Southern OB Stars",Astrophysical Journal,157:313–326,Bibcode:1969ApJ...157..313H,doi:10.1086/150069.
  4. ^abcdJilinski, E.; et al. (March 2006), "Radial velocity measurements of B stars in the Scorpius–Centaurus association",Astronomy and Astrophysics,448 (3):1001–1006,arXiv:astro-ph/0601643,Bibcode:2006A&A...448.1001J,doi:10.1051/0004-6361:20041614,S2CID 17818058.
  5. ^abcdTetzlaff, N.; et al. (2011), "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun",Monthly Notices of the Royal Astronomical Society,410 (1):190–200,arXiv:1007.4883,Bibcode:2011MNRAS.410..190T,doi:10.1111/j.1365-2966.2010.17434.x,S2CID 118629873.
  6. ^abcdeFitzpatrick, E. L.; Massa, D. (March 2005), "Determining the Physical Properties of the B Stars. II. Calibration of Synthetic Photometry",The Astronomical Journal,129 (3):1642–1662,arXiv:astro-ph/0412542,Bibcode:2005AJ....129.1642F,doi:10.1086/427855,S2CID 119512018.
  7. ^"ups01 Oph",SIMBAD,Centre de données astronomiques de Strasbourg, retrieved2019-10-21
  8. ^Eggleton, P. P.; Tokovinin, A. A. (2008), "A catalogue of multiplicity among bright stellar systems",Monthly Notices of the Royal Astronomical Society,389 (2): 869,arXiv:0806.2878,Bibcode:2008MNRAS.389..869E,doi:10.1111/j.1365-2966.2008.13596.x,S2CID 14878976.
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