Evidence of an asymmetrical Keplerian disk in the Br γ and He i emission lines around the Be star HD 110432

Astronomy and Astrophysics

Volumn 550, Issue , 2013, Pages

  Stee, Ph ^a   Meilland, A ^a,b   Bendjoya, Ph ^a   Millour, F ^a   Smith, M ^c   Spang, A ^a   Duvert, G ^d   Hofmann, K H ^e   Massi, F ^f  

^a UNIVERSITÉ DE NICE SOPHIA ANTIPOLIS   (France)

^b UNIVERSITY OF WESTERN ONTARIO   (Canada)

^c CATHOLIC UNIVERSITY OF AMERICA   (United States)

^d LABORATOIRE D ASTROPHYSIQUE   (France)

^e MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^f INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

Author keywords

Circumstellar matter; Instrumentation: interferometers; Stars: emission line, Be; Stars: individual: HD 110432; Stars: winds, outflows

Indexed keywords

CIRCUMSTELLAR MATTERS; INSTRUMENTATION: INTERFEROMETERS; STARS: EMISSION-LINE , BE; STARS: INDIVIDUAL; STARS: WINDS , OUTFLOWS;

X RAYS;

STARS;

EID: 84872912555     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201220302     Document Type: Article

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