The orbit of the close spectroscopic binary ε Lup and the intrinsic variability of its early B-type components

Astronomy and Astrophysics

Volumn 440, Issue 1, 2005, Pages 249-260

  Uytterhoeven, K ^a,b   Harmanec, P ^b,c   Telting, J H ^d   Aerts, C ^a,e  

^a UNIVERSITY OF LEUVEN   (Belgium)

^b ASTRONOMICAL INSTITUTE   (Czech Republic)

^c CHARLES UNIVERSITY   (Czech Republic)

^d NORDIC OPTICAL TELESCOPE   (Spain)

^e RADBOUD UNIVERSITY NIJMEGEN   (Netherlands)

Author keywords

Line: profiles; Stars: binaries: close; Stars: binaries: spectroscopic; Stars: individual: Lup; Stars: oscillations

Indexed keywords

ASTRONOMY; NATURAL FREQUENCIES; PARAMETER ESTIMATION; PULSE AMPLITUDE MODULATION; SPECTROSCOPIC ANALYSIS;

LINE: PROFILES; STARS: BINARIES: CLOSE; STARS: BINARIES: SPECTROSCOPIC; STARS: INDIVIDUAL: Ε LUP; STARS: OSCILLATIONS;

ORBITAL LABORATORIES;

EID: 24944451357     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20053009     Document Type: Article

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