Gyrosynchrotron Emission from Stellar Coronae

Details Gyrosynchrotron Emission from Stellar Coronae Gyrosynchrotron Emission from Stellar Coronae

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000iaus..195..393g&link_type=abstract

Highly Energetic Physical Processes and Mechanisms for Emission from Astrophysical Plasmas, Proceedings of IAU Symposium #195, h

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

We analyze quiescent radio spectra of main-sequence cool stars in terms
of a simple gyrosynchrotron model. We find that the underlying (assumed)
power-law electron distribution is often very hard, with power-law
indices (in dN / dE ~E-δ) mostly around δ
~2--3.5.

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