V945 Centauri = HD 112409: A bright hot short-period binary in a triple system?

Astronomy and Astrophysics

Volumn 520, Issue 10, 2010, Pages

  Harmanec, P ^a   Aerts, C ^b,c   Prsa A ^d,e   Verhoelst, T ^b   Kolenberg, K ^b,f  

^a CHARLES UNIVERSITY   (Czech Republic)

^b KU LEUVEN   (Belgium)

^c RADBOUD UNIVERSITY NIJMEGEN   (Netherlands)

^d VILLANOVA UNIVERSITY   (United States)

^e UNIVERSITY OF LJUBLJANA   (Slovenia)

^f UNIVERSITY OF VIENNA   (Austria)

Author keywords

binaries: close; stars: individual: V945 Cen = HD 112409; stars: variables: general

Indexed keywords

SPECTROSCOPIC ANALYSIS; SPECTROSCOPY;

BINARIES: CLOSE; CIRCULAR ORBIT; HIGH-RESOLUTION ECHELLE SPECTROSCOPY; HIPPARCOS DATA; OPTICAL SPECTRA; ORBITAL PERIODS; SPECTRAL LINE; SPECTRAL OBSERVATIONS; SPECTRAL TYPES; SPECTROSCOPIC BINARY; STARS: INDIVIDUAL: V945 CEN = HD 112409; STARS: VARIABLES: GENERAL; THIRD BODY; TRIPLE SYSTEM;

STARS;

EID: 77957697553     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014096     Document Type: Article

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