On the nature of the H i infrared emission lines of τ Scorpii

Astronomy and Astrophysics

Volumn 349, Issue 2, 1999, Pages 573-587

  Zaal, P A ^a   De Koter, A ^a   Waters, L B F M ^a,b   Maryborough, J M ^c   Geballe, T R ^d   Oliveira, J M ^e,f   Foing, B H ^e  

^a UNIVERSITY OF AMSTERDAM   (Netherlands)

^b SRON NETHERLANDS INSTITUTE FOR SPACE RESEARCH   (Netherlands)

^c UNIVERSITY OF WESTERN ONTARIO   (Canada)

^d UNIVERSITY OF HAWAII   (United States)

^e EUROPEAN SPACE AGENCY   (Netherlands)

^f CENTRO DE ASTROFÍSICA   (Portugal)

Author keywords

Infrared; stars; Line, be; Line: formation; Radiative transfer; Stars: atmospheres; Stars: emission; Stars; early type

Indexed keywords

EID: 0012839849     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

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