Magnetic topology and surface differential rotation on the K1 subgiant of the RS CVn system HR 1099

Monthly Notices of the Royal Astronomical Society

Volumn 348, Issue 4, 2004, Pages 1175-1190

  Petit, P ^a,b   Donati, J F ^a   Wade, G A ^c   Landstreet, J D ^d   Bagnulo, S ^e   Luftinger T ^f   Sigut, T A A ^d   Shorlin, S L S ^d   Strasser, S ^g   Auriere M ^a   Oliveira, J M ^h  

^a OBSERVATOIRE MIDI PYRÉNÉES   (France)

^b CENTRO DE ASTROFÍSICA   (Portugal)

^c ROYAL MILITARY COLLEGE OF CANADA   (Canada)

^d UNIVERSITY OF WESTERN ONTARIO   (Canada)

^e EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^f Institut fur Astronomie Vienna   (Austria)

^g UNIVERSITY OF CALGARY   (Canada)

^h KEELE UNIVERSITY   (United Kingdom)

Author keywords

Binaries: close; Polarization; Stars: activity; Stars: imaging; Stars: magnetic fields; Stars: rotation

Indexed keywords

MAGNETIC FIELDS; ROTATION RATE; STARS; TELESCOPES; TOPOLOGY;

BINARIES: CLOSE; CONVECTIVE ZONE; DIFFERENTIAL ROTATION; HR 1099; MAGNETIC TOPOLOGIES; STAR: ACTIVITY; STARS: MAGNETIC FIELD; STARS: ROTATION; STARS:IMAGING; SURFACE DIFFERENTIALS;

LUMINANCE;

EID: 1642296373     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.07420.x     Document Type: Article

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