Observations of Mira stars with the IOTA/FLUOR interferometer and comparison with Mira star models

New Astronomy

Volumn 7, Issue 1, 2002, Pages 9-20

  Hofmann, K H ^a   Beckmann, U ^a   Blocker T ^a   Coude du Foresto V ^b   Lacasse, M ^c   Mennesson, B ^b   Millan Gabet, R ^c   Morel, S ^c   Perrin, G ^b   Pras, B ^c   Ruilier, C ^b   Schertl, D ^a   Scholler M ^g   Scholz, M ^d,e   Shenavrin, V ^f   Traub, W ^c   Weigelt, G ^a   Wittkowski, M ^g   Yudin, B ^f  

^a MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^b OBSERVATOIRE DE PARIS   (France)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d UNIVERSITY OF HEIDELBERG   (Germany)

^e UNIVERSITY OF SYDNEY   (Australia)

^f MOSCOW STATE UNIVERSITY   (Russian Federation)

^g ESO   (Germany)

Author keywords

Instrumentation: Interferometers; Stars: AGB and post AGB; Stars: Individual: R Aql; Stars: Individual: R Ser; Stars: Individual: RU her; Stars: Individual: V CrB; Stars: Individual: X Oph; Stars: Late type; Stars: Variables

Indexed keywords

EID: 31244434700     PISSN: 13841076     EISSN: None     Source Type: Journal    
DOI: 10.1016/S1384-1076(01)00085-9     Document Type: Article

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