An improved method for the determination of the orbital parameters of a binary system that contains a pulsating component

Astronomy and Astrophysics Supplement Series

Volumn 135, Issue 2, 1999, Pages 383-390

  Molenberghs, G ^a   Aerts, C ^b,c   De Cat, P ^b  

^a HASSELT UNIVERSITY   (Belgium)

^b KU LEUVEN   (Belgium)

^c FUND FOR SCIENTIFIC RESEARCH   (Belgium)

Author keywords

Binaries: spectroscopic; Methods: statistical; Stars: oscillations

Indexed keywords

EID: 16644396570     PISSN: 03650138     EISSN: None     Source Type: Journal    
DOI: 10.1051/aas:1999180     Document Type: Article

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