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Nonthermal Microwave Phenomena in Other Stars

Published online by Cambridge University Press:  14 August 2015

R. M. Hjellming  and
D. M. Gibson
R. M. Hjellming
Affiliation:
National Radio Astronomy Observatory*, Socorro, NM
D. M. Gibson
Affiliation:
New Mexico Institute of Mining and Technology, Socorro, NM

Abstract

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Several classes of “normal” stellar objects exhibit microwave phenomena, predominantly at cm wavelengths. These include RS CVn binaries, Algol-type binaries, M supergiants, and UV Ceti-type flare stars. The emission mechanisms are generally either synchrotron or gryosynchrotron radiation, with the latter being predominant in the numerous RS CVn radio emitters which sometimes exhibit variable circular polarization. “Events” have time scales varying from minutes to days.

Type
Session III - Solar Bursts - cm Wavelengths
Information
Symposium - International Astronomical Union , Volume 86: Radio Physics of the Sun , 1980 , pp. 209 - 220
Copyright
Copyright © Reidel 1980 

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