Magnetic fields and differential rotation on the pre-main sequence -I. The early-G star HD 141943 - brightness and magnetic topologies

Monthly Notices of the Royal Astronomical Society

Volumn 413, Issue 3, 2011, Pages 1922-1938

  Marsden, S C ^a,b   Jardine, M M ^c   Ramirez Velez J C ^d,e   Alecian, E ^d,f   Brown, C J ^g   Carter, B D ^g   Donati, J F ^h   Dunstone, N ^c   Hart, R ^g   Semel, M ^d   Waite, I A ^g  

^a JAMES COOK UNIVERSITY   (Australia)

^b AUSTRALIAN ASTRONOMICAL OBSERVATORY   (Australia)

^c UNIVERSITY OF ST ANDREWS   (United Kingdom)

^d UNIVERSITÉ PARIS DIDEROT   (France)

^e UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

^f UNIV GRENOBLE ALPES   (France)

^g UNIVERSITY OF SOUTHERN QUEENSLAND   (Australia)

^h UNIVERSITÉ DE TOULOUSE   (France)

Author keywords

Line: profiles; Magnetic fields; Stars: activity; Stars: imaging; Stars: individual: HD 141943; Starspots

Indexed keywords

LUMINANCE; SIGNAL TO NOISE RATIO; STARS; TOPOLOGY;

LINE: PROFILES; MAGNETIC TOPOLOGIES; MAGNETIC-FIELD; PRE-MAIN SEQUENCES; STAR: ACTIVITY; STAR: INDIVIDUAL: HD 141943; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS:IMAGING; STARSPOTS; SURFACE MAGNETIC FIELD;

MAGNETIC FIELDS;

EID: 79955766031     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2011.18367.x     Document Type: Article

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