Magnetic fields and accretion flows on the classical T Tauri star V2129 Oph

Monthly Notices of the Royal Astronomical Society

Volumn 380, Issue 4, 2007, Pages 1297-1312

  Donati, J F ^a   Jardine, M M ^b   Gregory, S G ^b   Petit, P ^a   Bouvier, J ^c   Dougados, C ^c   Menard F ^c   Cameron, A C ^b   Harries, T J ^d   Jeffers, S V ^a,e   Paletou, F ^a  

^a OBSERVATOIRE MIDI PYRÉNÉES   (France)

^b UNIVERSITY OF ST ANDREWS   (United Kingdom)

^c UNIVERSITÉ MONTPELLIER 2   (France)

^d UNIVERSITY OF EXETER   (United Kingdom)

^e UTRECHT UNIVERSITY   (Netherlands)

Author keywords

Accretion, accretion discs; Stars: formation; Stars: individual: V2129 Oph; Stars: magnetic fields; Stars: rotation; Techniques: spectroscopic

Indexed keywords

MAGNETIC FIELDS; MODULATION; ROTATION; STARS; TOPOLOGY;

ACCRETION: ACCRETION DISKS; LARGE-SCALES; MAGNETIC-FIELD; STAR: INDIVIDUAL: V2129 OPH; STARS FORMATION; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: MAGNETIC FIELD; STARS: ROTATION; T TAURI STARS; TECHNIQUES: SPECTROSCOPIC;

MAGNETOSPHERE;

EID: 34748910577     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.12194.x     Document Type: Article

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