Unveiling mira stars behind the molecules confirmation of the molecular layer model with narrow band near-infrared interferometry

Astronomy and Astrophysics

Volumn 426, Issue 1, 2004, Pages 279-296

  Perrin, G ^a   Ridgway, S T ^a,b   Mennesson, B ^c   Cotton, W D ^d   Woillez, J ^a,e   Verhoelst, T ^a,f   Schuller, P ^g   Coude Du Foresto V ^a   Traub, W A ^g   Millan Gabet, R ^h   Lacasse, M G ^g  

^a OBSERVATOIRE DE PARIS   (France)

^b NATIONAL OPTICAL ASTRONOMY OBSERVATORY   (United States)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^d NATIONAL RADIO ASTRONOMY OBSERVATORY   (United States)

^e Keck Observatory   (United States)

^f Sterrenkunde Leuven   (Belgium)

^g HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^h CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

Infared: stars; Stars: AGB and post AGB; Stars: fundamental parameters; Stars: mass loss; Techniques: Interferometric

Indexed keywords

CARBON MONOXIDE; CHARACTERIZATION; IMAGE ANALYSIS; INTERFEROMETERS; INTERFEROMETRY; SPECTROSCOPIC ANALYSIS; WATER;

MOLECULAR BANDS; MOLECULAR LAYERS; NARROW BANDS; STARS; WATER VAPORS;

ASTROPHYSICS;

EID: 6344280618     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20041098     Document Type: Article

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