Non-thermal radio emission from O-type stars III. Is Cygnus OB2 No. 9 a wind-colliding binary?

Astronomy and Astrophysics

Volumn 483, Issue 2, 2008, Pages 585-590

  Van Loo, S ^a   Blomme, R ^b   Dougherty, S M ^c   Runacres, M C ^d  

^a UNIVERSITY OF LEEDS   (United Kingdom)

^b ROYAL OBSERVATORY OF BELGIUM   (Belgium)

^c NATIONAL RESEARCH COUNCIL CANADA   (Canada)

^d Erasmus University College   (Belgium)

Author keywords

Radiation mechanisms: non thermal; Stars: early type; Stars: individual: Cyg OB2 No. 9; Stars: mass loss

Indexed keywords

PARAMETER ESTIMATION; RADIO WAVES; SPECTROSCOPIC ANALYSIS;

MASS LOSS; RADIATION MECHANISMS; RADIO EMISSION; THERMAL EMISSION; WIND COLLISION REGION;

STARS;

EID: 43249122471     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200809367     Document Type: Article

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