3D models of radiatively driven colliding winds in massive O + O star binaries - II. Thermal radio to submillimetre emission

Monthly Notices of the Royal Astronomical Society

Volumn 403, Issue 4, 2010, Pages 1633-1656

  Pittard, J M ^a  

^a UNIVERSITY OF LEEDS   (United Kingdom)

Author keywords

Binaries: general; Radio continuum: stars; Shock waves; Stars: early type; Stars: mass loss; Stars: winds, outflows

Indexed keywords

SHOCK WAVES; STARS;

BINARIES:GENERAL; COLLISION REGION; RADIO CONTINUUM: STARS; SHOCK-WAVES; STARS: BINARIES; STARS: MASS-LOSS; STARS: WINDS OUTFLOWS; STARS:EARLY TYPE; SUBMILLIMETRE; THERMAL EMISSIONS;

WIND;

EID: 77953040858     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2010.15516.x     Document Type: Article

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