Confirmation of the magnetic oblique rotator model for the Of?p star HD191612

Monthly Notices of the Royal Astronomical Society

Volumn 416, Issue 4, 2011, Pages 3160-3169

  Wade, G A ^a   Howarth, I D ^b   Townsend, R H D ^c   Grunhut, J H ^a,d   Shultz, M ^a,d   Bouret, J C ^e,f   Fullerton, A ^g   Marcolino, W ^h   Martins, F ⁱ   Naze Y ^j   ud Doula, A ^k   Walborn, N R ^g   Donati, J F ^l  

^a ROYAL MILITARY COLLEGE OF CANADA   (Canada)

^b UNIVERSITY COLLEGE LONDON   (United Kingdom)

^c UNIVERSITY OF WISCONSIN MADISON   (United States)

^d QUEEN S UNIVERSITY   (Canada)

^e AIX MARSEILLE UNIVERSITÉ   (France)

^f NASA GODDARD SPACE FLIGHT CENTER   (United States)

^g STScI   (United States)

^h FEDERAL UNIVERSITY OF RIO DE JANEIRO   (Brazil)

ⁱ UNIVERSITÉ MONTPELLIER II   (France)

^j UNIVERSITY OF LIÈGE   (Belgium)

^k PENNSYLVANIA STATE UNIVERSITY   (United States)

^l OBSERVATOIRE MIDI PYRÉNÉES   (France)

more..

Author keywords

Stars: individual: HD 191612; Stars: magnetic field; Stars: massive; Stars: rotation

Indexed keywords

MAGNETIC FIELDS; MAGNETOPLASMA; MAGNETOSPHERE; PHOTOMETRY; PLASMA DENSITY;

EQUIVALENT WIDTH; LONGITUDINAL FIELDS; MAGNETIC-FIELD; MAGNETOSPHERICS; ORBITALS; STAR: INDIVIDUAL: HD 191612; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: MAGNETIC FIELD; STARS: MASSIVE; STARS: ROTATION;

STARS;

EID: 80052961887     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2011.19265.x     Document Type: Article

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