Non-thermal emission in Wolf-Rayet stars: Are massive companions required?

Monthly Notices of the Royal Astronomical Society

Volumn 319, Issue 4, 2000, Pages 1005-1010

  Dougherty, S M ^a,b   Williams, P M ^c  

^a NATIONAL RESEARCH COUNCIL CANADA   (Canada)

^b UNIVERSITY OF CALGARY   (Canada)

^c UNIVERSITY OF EDINBURGH   (United Kingdom)

Author keywords

Radio continuum: stars; Stars: Individual: WR 86; Stars: Wolf Rayet

Indexed keywords

COLLISION REGION; NONTHERMAL EMISSION; RADIO CONTINUUM: STARS; STAR: INDIVIDUAL: WOLF-RAYET 86; STARS: BE; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: WOLF-RAYET; STELLAR WIND; WOLF-RAYET; WOLF-RAYET STARS;

STARS;

EID: 0000860456     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2000.03837.x     Document Type: Article

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