HR5907: Discovery of the most rapidly rotating magnetic early B-type star by the MiMeS Collaboration†

Monthly Notices of the Royal Astronomical Society

Volumn 419, Issue 2, 2012, Pages 1610-1627

  Grunhut, J H ^a,b   Rivinius, Th ^c   Wade, G A ^b   Townsend, R H D ^d   Marcolino, W L F ^e   Bohlender, D A ^f   Szeifert, Th ^c   Petit, V ^g   Matthews, J M ^h   Rowe, J F ⁱ   Moffat, A F J ^j   Kallinger, T ^h,k   Kuschnig, R ^h,k   Guenther, D B ^l   Rucinski, S M ^m   Sasselov, D ⁿ   Weiss, W W ^l  

^a QUEEN S UNIVERSITY   (Canada)

^b ROYAL MILITARY COLLEGE OF CANADA   (Canada)

^c EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^d UNIVERSITY OF WISCONSIN MADISON   (United States)

^e FEDERAL UNIVERSITY OF RIO DE JANEIRO   (Brazil)

^f NATIONAL RESEARCH COUNCIL CANADA   (Canada)

^g WEST CHESTER UNIVERSITY   (United States)

^h UNIVERSITY OF BRITISH COLUMBIA   (Canada)

ⁱ NASA AMES RESEARCH CENTER   (United States)

^j UNIVERSITÉ DE MONTRÉAL   (Canada)

^k UNIVERSITY OF VIENNA   (Austria)

^l SAINT MARY S UNIVERSITY   (Canada)

^m UNIVERSITY OF TORONTO   (Canada)

ⁿ HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

more..

Author keywords

Stars: circumstellar matter; Stars: individual HR5907; Stars: magnetic field; Stars: rotation; Techniques: photometric; Techniques: polarimetric

Indexed keywords

EID: 83855162754     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2011.19824.x     Document Type: Article

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