A three-dimensional model for the radio emission of magnetic chemically peculiar stars

Astronomy and Astrophysics

Volumn 418, Issue 2, 2004, Pages 593-605

  Trigilio, C ^a   Leto, P ^a   Umana, G ^a   Leone, F ^b   Buemi, C S ^a  

^a CNR   (Italy)

^b INAF OSSERVATORIO ASTROFISICO DI TORINO   (Italy)

Author keywords

Radio continuum: stars; Stars: chemically peculiar; Stars: circumstellar matter; Stars: individual: HD 37479, HD 37017; Stars: magnetic field

Indexed keywords

ASTROPHYSICS; COMPUTER SIMULATION; DEFORMATION; ELECTROMAGNETIC WAVE ABSORPTION; ELECTROMAGNETIC WAVE EMISSION; ELECTRON EMISSION; MAGNETIC FIELD EFFECTS; MAGNETOSPHERE; SPECTRUM ANALYSIS; ULTRAVIOLET RADIATION; X RAYS;

CHEMICALLY PECULIAR STARS; GYROSYNCHROTRON EMITTING REGION; HD 37017; HD 37479 STARS; MAGNETIC FIELD RADIO CONTINUUM; STELLAR WINDS;

RADIO ASTRONOMY;

EID: 2142837164     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20040060     Document Type: Article

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