Multiple star system in the constellation of Lupus
Mu Lupi (μ Lup ) is a system of three or four stars in the southern constellation of Lupus . It is visible to the naked eye with an apparent visual magnitude of 4.29 and lies roughly 340 light-years from the Sun .
Two of the components of this system, A and B, form a pair with an angular separation of 1.1 arcseconds . As of 2014, no orbit has been published. Component C lies at an angular separation of 22.6 arcseconds from the AB pair, and may be a common proper motion companion. It is an A-type main-sequence star with a classification of A2 V. A fourth component at an angular separation of 6.15 arcseconds from component A, may be a brown dwarf .
References
^ 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 , S2CID 18759600 .
^ Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalogue of Eggen's UBV Data , SIMBAD , Bibcode :1986EgUBV........0M .
^ Levenhagen, R. S.; Leister, N. V. (2006), "Spectroscopic analysis of southern B and Be stars", Monthly Notices of the Royal Astronomical Society , 371 (1): 252–262, arXiv :astro-ph/0606149 , Bibcode :2006MNRAS.371..252L , doi :10.1111/j.1365-2966.2006.10655.x , S2CID 16492030 .
de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project", Astronomy & Astrophysics , 546 : 14, arXiv :1208.3048 , Bibcode :2012A&A...546A..61D , doi :10.1051/0004-6361/201219219 , S2CID 59451347 , A61.
Hubrig, S.; et al. (June 2001), "Search for low-mass PMS companions around X-ray selected late B stars", Astronomy and Astrophysics , 372 : 152–164, arXiv :astro-ph/0103201 , Bibcode :2001A&A...372..152H , doi :10.1051/0004-6361:20010452 , S2CID 17507782 .
"* mu. Lup -- Be Star" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2017-03-08.{{cite web }}
: CS1 maint: postscript (link )
^ Veramendi, M. E.; González, J. F. (July 2014), "Spectroscopic study of early-type multiple stellar systems. II. New binary subsystems", Astronomy & Astrophysics , 567 : 10, arXiv :1405.1084 , Bibcode :2014A&A...567A..35V , doi :10.1051/0004-6361/201423736 , S2CID 21711755 , A35.
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