Non-thermal radio emission from O-type stars I. HD 168112

Astronomy and Astrophysics

Volumn 436, Issue 3, 2005, Pages 1033-1040

  Blomme, R ^a   Van Loo, S ^a   De Becker, M ^b   Rauw, G ^b   Runacres, M C ^a   Setia Gunawan, D Y A ^c   Chapman, J M ^c  

^a ROYAL OBSERVATORY OF BELGIUM   (Belgium)

^b UNIVERSITY OF LIÈGE   (Belgium)

^c CSIRO   (Australia)

Author keywords

Radiation mechanisms: non thermal; Radio continuum: stars; Stars: early type; Stars: individual: HD 168112; Stars: mass loss; Stars: winds, outflows

Indexed keywords

ASTROPHYSICS; ELECTRONS; EMISSION SPECTROSCOPY; FERMI LEVEL; GALAXIES; RADIATION EFFECTS; SYNCHROTRON RADIATION; X RAYS;

RADIATION MECHANISMS:NON-THERMAL; RADIO CONTINUUM:STARS; STARS:EARLY-TYPE; STARS:INDIVIDUAL:HD 168112; STARS:MASS-LOSS; STARS:WINDS, OUTFLOWS;

RADIO ASTRONOMY;

EID: 21244477866     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20042383     Document Type: Article

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