An investigation of the magnetic properties of the classical Be star ω Ori by the MiMeS Collaboration

Monthly Notices of the Royal Astronomical Society

Volumn 426, Issue 4, 2012, Pages 2738-2750

  Neiner, C ^a   Grunhut, J H ^b,c   Petit, V ^d   Ud Doula, A ^e   Wade, G A ^c   Landstreet, J ^f   de Batz, B ^a   Cochard, F ^g   Gutierrez Soto J ^h,i   Huat, A L ^j  

^a UNIVERSITÉ PARIS DIDEROT   (France)

^b QUEEN S UNIVERSITY   (Canada)

^c ROYAL MILITARY COLLEGE OF CANADA   (Canada)

^d WEST CHESTER UNIVERSITY   (United States)

^e PENNSYLVANIA STATE UNIVERSITY   (United States)

^f UNIVERSITY OF WESTERN ONTARIO   (Canada)

^g Shelyak Instruments   (France)

^h VALENCIAN INTERNATIONAL UNIVERSITY   (Spain)

ⁱ INSTITUTO DE ASTROFÍSICA DE ANDALUCÍA CSIC   (Spain)

^j UNIVERSITÉ PARIS DIDEROT   (France)

more..

Author keywords

Circumstellar matter; Stars: emission line, Be; Stars: individual: Ori; Stars: magnetic field

Indexed keywords

EID: 84867867712     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2012.21833.x     Document Type: Article

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