Long-term spectroscopic monitoring of BA-type supergiants: III. Variability of photospheric lines

Astronomy and Astrophysics

Volumn 320, Issue 1, 1997, Pages 273-286

  Kaufer, A ^a   Stahl, O ^a   Wolf, B ^a   Fullerton, A W ^d,e   Gang Th ^a,c   Gummersbach, C A ^a   Jankovics, I ^b   Kovacs J ^b   Mandel, H ^a   Peitz, J ^a   Rivinius, Th ^a   Szeifert, Th ^a  

^a UNIVERSITÄT HEIDELBERG   (Germany)

^b Gothard Astrophysical Observatory   (Hungary)

^c AURA for the European Space Agency   (United States)

^d MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^e UNIVERSITY OF MUNICH   (Germany)

Author keywords

Emission line; Pulsation; Rotation; Stars: early type; Supergiants

Indexed keywords

EID: 0012233440     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

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