Line-profile variations due to adiabatic non-radial pulsations in rotating stars. I. Observable characteristics of spheroidal modes

Astronomy and Astrophysics Supplement Series

Volumn 121, Issue 2, 1997, Pages 343-368

  Schrijvers, C ^a   Telting, J H ^a   Aerts, C ^b,d   Ruymaekers, E ^c   Henrichs, H F ^a  

^a UNIVERSITY OF AMSTERDAM   (Netherlands)

^b KU LEUVEN   (Belgium)

^c Belgian National Fund for Scientific Research ^*  (Belgium)

^d FUND FOR SCIENTIFIC RESEARCH   (Belgium)

Author keywords

Line: profiles; Stars: oscillations, rotation; Stars: variable: Sct stars; others

Indexed keywords

EID: 33745602688     PISSN: 03650138     EISSN: None     Source Type: Journal    
DOI: 10.1051/aas:1997321     Document Type: Article

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