The magnetic field and circumstellar environment of the helium-strong star HD 36485 = δ Ori C

Monthly Notices of the Royal Astronomical Society

Volumn 401, Issue 4, 2010, Pages 2739-2752

  Leone, F ^a   Bohlender, D A ^b   Bolton, C T ^c   Buemi, C ^d   Catanzaro, G ^d   Hill, G M ^e   Stift, M J ^f  

^a UNIVERSITY OF CATANIA   (Italy)

^b NATIONAL RESEARCH COUNCIL CANADA   (Canada)

^c UNIVERSITY OF TORONTO   (Canada)

^d INAF OSSERVATORIO ASTROFISICO DI CATANIA   (Italy)

^e W M KECK OBSERVATORY   (United States)

^f UNIVERSITY OF VIENNA   (Austria)

Author keywords

Binaries: spectroscopic; Circumstellar matter; Stars: chemically peculiar; Stars: individual: HD 36485; Stars: magnetic fields

Indexed keywords

HELIUM; MAGNETIC FIELDS; MAGNETOSPHERE; ROTATION; SPECTROSCOPIC ANALYSIS;

BINARIES: SPECTROSCOPIC; CIRCUMSTELLAR; CIRCUMSTELLAR MATTERS; HΑ EMISSION; MAGNETIC-FIELD; RADIAL VELOCITY MEASUREMENTS; STAR: INDIVIDUAL: HD 36485; STARS: CHEMICALLY PECULIAR; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: MAGNETIC FIELD;

STARS;

EID: 74549149559     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.15858.x     Document Type: Article

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