The molecular and dusty composition of Betelgeuse's inner circumstellar environment

Astronomy and Astrophysics

Volumn 474, Issue 2, 2007, Pages 599-608

  Perrin, G ^a   Verhoelst, T ^b,h   Ridgway, S T ^c   Cami, J ^d   Nguyen, Q N ^a   Chesneau, O ^e   Lopez, B ^e   Leinert, Ch ^f   Richichi, A ^g  

^a UNIVERSITÉ PARIS DIDEROT   (France)

^b KU LEUVEN   (Belgium)

^c NATIONAL OPTICAL ASTRONOMY OBSERVATORY   (United States)

^d UNIVERSITY OF WESTERN ONTARIO   (Canada)

^e UNIVERSITÉ CÔTE D'AZUR   (France)

^f MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^g EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^h FUND FOR SCIENTIFIC RESEARCH   (Belgium)

Author keywords

Stars: fundamental parameters; Stars: individual: Betelgeuse infrared: stars; Stars: mass loss; Techniques: interferometric

Indexed keywords

DUSTY COMPOSITION; GEOMETRIC MODEL; MASSIVE STARS; RED SUPERGIANT STARS;

ASTROPHYSICS; COMPUTATIONAL GEOMETRY; DATA REDUCTION; INFRARED SPECTROSCOPY; INTERFEROMETRY; PARAMETER ESTIMATION;

STARS;

EID: 35548944043     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20077863     Document Type: Article

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