Polarized light from lower main-sequence stars - Is it due to synchrotron emission

Details Polarized light from lower main-sequence stars - Is it due to synchrotron emission Polarized light from lower main-sequence stars - Is it due to synchrotron emission

Nov 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...201..630m&link_type=abstract

Astrophysical Journal, vol. 201, Nov. 1, 1975, pt. 1, p. 630-636.

Astronomy and Astrophysics

Astrophysics

2

Late Stars, Main Sequence Stars, Polarized Light, Stellar Radiation, Synchrotron Radiation, Variable Stars, Compton Effect, Electron Distribution, Electron Energy, Energy Spectra, Flares, Stellar Luminosity, Stellar Temperature

Scientific paper

Broadband plane polarization (0.1-10%) has been observed in the light emitted by flare stars outside flares. The possibility that the polarization might be due to synchrotron radiation is examined. On the basis of the electron energy spectrum which would be required, it is suggested that synchrotron radiation is probably not responsible for the observed polarization.

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