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Chi Lupi

From Wikipedia, the free encyclopedia
Star in the constellation Lupus
χ Lupi
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationLupus
Right ascension15h 50m 57.5376s[1]
Declination−33° 37′ 37.796″[1]
Apparent magnitude (V)3.957[1]
Characteristics
Spectral typeB9.5V + A2Vm[2]
U−Bcolor index−0.13[3]
B−Vcolor index−0.04[3]
R−Icolor index−0.07[3]
Astrometry
Radial velocity (Rv)5 ± 20[1] km/s
Proper motion (μ)RA: −5.92[1]mas/yr
Dec.: −24.91[1]mas/yr
Parallax (π)15.86±0.84 mas[1]
Distance210 ± 10 ly
(63 ± 3 pc)
Details[4]
χ Lup A
Mass2.84±0.12 M
Radius2.85±0.15 R
Luminosity63[5] L
Surface gravity (log g)4.08[5] cgs
Temperature10,200[5] K
Rotational velocity (v sin i)0[3] km/s
Age280±30 Myr
χ Lup B
Mass1.94±0.09 M
Radius1.75±0.18 R
Surface gravity (log g)4.2 cgs
Temperature9,200 K
Other designations
χ Lup, Chi Lupi, Chi Lup,5 Lupi, 5 Lup,CD−33 10754,CPD−33 3933,FK5 586,GC 21281,HD 141556,HIP 77634,HR 5883,PPM 294334,SAO 207040.[1]
Database references
SIMBADdata

Chi Lupi (Chi Lup,χ Lupi,χ Lup) is aspectroscopic binarystar in theconstellation ofLupus.[1] It has anapparent visual magnitude of approximately 3.957.[1] The primary star in the binary is amercury-manganese star of spectral type B9.5V; the secondary is ametallic-lined star of type A2Vm.[2]

This system is aproper motion member of the Upper Scorpius sub-group in theScorpius–CentaurusOB association,the nearest such co-moving association of massive stars to the Sun.[5]The Upper Scorpius subgroup contains thousands ofstars with an average age of 11 million years old at mean distances of 145parsecs (470light years).[6]

References

[edit]
  1. ^abcdefghij"chi Lup".SIMBAD.Centre de données astronomiques de Strasbourg. RetrievedAugust 14, 2008.
  2. ^abOn the Ga II and Ga III Resonance Lines and the Implication for Chemical Stratification in HgMn Stars, K. E. Nielsen et al.,Astronomical Journal130, #5 (November 2005), pp. 2312–2317,Bibcode:2005AJ....130.2312N,doi:10.1086/491703.
  3. ^abcdHR 5883, database entry, The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version), D. Hoffleit and W. H. Warren, Jr.,CDS IDV/50. Accessed on line August 14, 2008.
  4. ^Le Bouquin, J.-B.; Beust, H.; Duvert, G.; Berger, J. P.; Ménard, F.; Zins, G. (March 2013), "Masses and age of the chemically peculiar double-lined binary χ Lupi",Astronomy & Astrophysics,551: 9,arXiv:1302.5014,Bibcode:2013A&A...551A.121L,doi:10.1051/0004-6361/201220454,S2CID 13860888, A121.
  5. ^abcdde Geus, E. J.; de Zeeuw, P. T.; Lub, J. (June 1989), "Physical parameters of stars in the Scorpio-Centaurus OB association",Astronomy and Astrophysics,216 (1–2):44–61,Bibcode:1989A&A...216...44D
  6. ^Mark J. Pecaut; Eric E. Mamajek & Eric J. Bubar (February 2012). "A Revised Age for Upper Scorpius and the Star Formation History among the F-type Members of the Scorpius–Centaurus OB Association".Astrophysical Journal.746 (2): 154.arXiv:1112.1695.Bibcode:2012ApJ...746..154P.doi:10.1088/0004-637X/746/2/154.S2CID 118461108.
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