The variable radio emission from magnetic chemically peculiar stars

Details The variable radio emission from magnetic chemically peculiar stars The variable radio emission from magnetic chemically peculiar stars

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...252..198l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 252, no. 1, Dec. 1991, p. 198-202.

Astronomy and Astrophysics

Astrophysics

14

Peculiar Stars, Radio Stars, Stellar Magnetic Fields, Variable Stars, Cosmochemistry, Stellar Mass, Stellar Radiation, Stellar Winds, Synchrotron Radiation

Scientific paper

Radio emission from chemically peculiar stars, detected by Drake et al. (1987), shows evidence of variability with the period of the light, spectrum and magnetic field variations. The possibility that such periodic radio emission is gyroradiation from the electron component of the wind, which flows along the open lines of the magnetic field, is numerically explored.

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