Improved estimates of the physical properties of the O-star binary V1007 Sco = HD 152248 and notes on several other binaries in the NGC 6231 cluster

Astronomy and Astrophysics

Volumn 481, Issue 1, 2008, Pages 183-192

  Mayer, P ^a   Harmanec, P ^a   Nesslinger, S ^b   Lorenz, R ^b   Drechsel, H ^b   Morrell, N ^c   Wolf, M ^a  

^a CHARLES UNIVERSITY   (Czech Republic)

^b UNIVERSITY OF ERLANGEN NUREMBERG   (Germany)

^c LAS CAMPANAS OBSERVATORY   (Chile)

Author keywords

Binaries: eclipsing; Stars: early type; Stars: emission line, Be; Stars: fundamental parameters; Stars: individual: V1007 Sco

Indexed keywords

ASTROPHYSICS; ATMOSPHERIC SPECTRA; GALAXIES; MATHEMATICAL MODELS; ORBITS; PHOTOMETRY;

BINARIES: ECLIPSING; STARS: EARLY-TYPE; STARS: EMISSION-LINE, BE; STARS: FUNDAMENTAL PARAMETERS; STARS: INDIVIDUAL: V1007 SCO;

STARS;

EID: 41449089993     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20078542     Document Type: Article

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