Article (Scientific journals)
Absolute dimensions of eclipsing binaries. XIV - UX Mensae
Andersen, J.; Clausen, J. V.; Magain, Pierre
1989In Astronomy and Astrophysics, 211, p. 346-352
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Keywords :
ECLIPSING BINARY STARS; STELLAR EVOLUTION; STELLAR LUMINOSITY; STELLAR MASS; ASTRONOMICAL PHOTOMETRY; LIGHT CURVE; METALLICITY; RADIAL VELOCITY; RADII; STELLAR ORBITS
Abstract :
[en] Spectroscopic orbits are determined for the 4-day, F8 V eclipsing binary UX Mensae. The masses of the binary components are 1.24 and 1.20 solar masses with errors of + or - 0.5 percent. The results of the analysis of the uvby light curves by Clausen and Gronbech (1976) are confirmed. The metal abundance is found to be Fe/H = +0.04 + or - 0.10. Absolute dimensions are computed for the binary. Theoretical evolutionary sequences for the masses and metal abundance are interpolated from the models of VandenBerg (1988) and Andersen et al. (1988).
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Andersen, J.;  Universitetets Astronomiske Observatorium, Tollose, Denmark ; Harvard-Smithsonian Center for Astrophysics, Cambridge, MA
Clausen, J. V.;  Universitetets Astronomiske Observatorium, Tollose, Denmark
Magain, Pierre  ;  Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique et traitement de l'image
Language :
English
Title :
Absolute dimensions of eclipsing binaries. XIV - UX Mensae
Publication date :
01 March 1989
Journal title :
Astronomy and Astrophysics
ISSN :
0004-6361
eISSN :
1432-0746
Publisher :
EDP Sciences, Les Ulis, France
Volume :
211
Pages :
346-352
Peer reviewed :
Peer Reviewed verified by ORBi
Available on ORBi :
since 02 February 2010

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