The close classical T Tauri binary V4046 Sgr: Complex magnetic fields and distributed mass accretion

Monthly Notices of the Royal Astronomical Society

Volumn 417, Issue 3, 2011, Pages 1747-1759

  Donati, J F ^a   Gregory, S G ^b   Montmerle, T ^c,d   Maggio, A ^e   Argiroffi, C ^e,f   Sacco, G ^g   Hussain, G ^h   Kastner, J ^g   Alencar, S H P ⁱ   Audard, M ^j   Bouvier, J ^d   Damiani, F ^e   Gudel M ^k   Huenemoerder, D ^l   Wade, G A ^m  

^a UNIVERSITÉ DE TOULOUSE   (France)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^c INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^d LABORATOIRE D ASTROPHYSIQUE   (France)

^e INAF OSSERVATORIO ASTROFISICO DI TORINO   (Italy)

^f UNIVERSITY OF PALERMO   (Italy)

^g ROCHESTER INSTITUTE OF TECHNOLOGY   (United States)

^h EUROPEAN SOUTHERN OBSERVATORY   (Germany)

ⁱ FEDERAL UNIVERSITY OF MINAS GERAIS   (Brazil)

^j UNIVERSITY OF GENEVA   (Switzerland)

^k UNIVERSITY OF VIENNA   (Austria)

^l MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^m ROYAL MILITARY COLLEGE OF CANADA   (Canada)

more..

Author keywords

Stars: formation; Stars: imaging; Stars: individual: V4046 Sgr; Stars: magnetic fields; Stars: rotation; Techniques: polarimetric

Indexed keywords

EID: 80055120102     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2011.19366.x     Document Type: Article

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