Magnetic fields and chemical peculiarities of the very young intermediate-mass binary system HD 72106

Monthly Notices of the Royal Astronomical Society

Volumn 391, Issue 2, 2008, Pages 901-914

  Folsom, C P ^a,b,c   Wade, G A ^a   Kochukhov, O ^d   Alecian, E ^a   Catala, C ^e   Bagnulo, S ^c   Bohm T ^f   Bouret, J C ^g   Donati, J F ^f   Grunhut, J ^a,b   Hanes, D A ^b   Landstreet, J D ^h  

^a ROYAL MILITARY COLLEGE OF CANADA   (Canada)

^b QUEEN S UNIVERSITY   (Canada)

^c ARMAGH OBSERVATORY   (United Kingdom)

^d UPPSALA UNIVERSITY   (Sweden)

^e OBSERVATOIRE DE PARIS   (France)

^f OBSERVATOIRE MIDI PYRÉNÉES   (France)

^g AIX MARSEILLE UNIVERSITÉ   (France)

^h UNIVERSITY OF WESTERN ONTARIO   (Canada)

Author keywords

Stars: abundances; Stars: chemically peculiar; Stars: evolution; Stars: individual: HD 72106; Stars: magnetic fields

Indexed keywords

CHEMICAL ANALYSIS; CHROMIUM; GEOMETRY; IRON; MAGNETIC FIELDS; POPULATION DISTRIBUTION; SYSTEMS (METALLURGICAL);

BE STARS; BINARY SYSTEMS; MAGNETIC-FIELD; MAGNETIC-FIELD GEOMETRY; STAR: EVOLUTION; STAR: INDIVIDUAL: HD 72106; STARS ABUNDANCES; STARS: CHEMICALLY PECULIAR; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: MAGNETIC FIELD;

STARS;

EID: 57149142412     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.13946.x     Document Type: Article

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