Hα emission line spectroscopy in NGC 330. On the hybrid model for global oscillations in Be star circumstellar disks

Astronomy and Astrophysics

Volumn 371, Issue 3, 2001, Pages 932-942

  Hummel, W ^a,b   Gassler W ^a,c   Muschielok, B ^a   Schink, H ^d   Nicklas, H ^d   Conti, G ^e   Mattaini, E ^e   Keller, S ^f   Mantel, K H ^a   Appenzeller, I ^g   Rupprecht, G ^b   Seifert, W ^g   Stahl, O ^g   Tarantik, K ^a,h  

^a UNIVERSITY OF MUNICH   (Germany)

^b EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^c NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^d UNIVERSITY OF GÖTTINGEN   (Germany)

^e CNR   (Italy)

^f AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^g UNIVERSITÄT HEIDELBERG   (Germany)

^h MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

Author keywords

Line: formation, profiles; Stars: circumstellar matter, emission line, Be

Indexed keywords

EID: 0035355259     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20010386     Document Type: Article

References (53)