Synchrotron emission from chaotic stellar winds

Details Synchrotron emission from chaotic stellar winds Synchrotron emission from chaotic stellar winds

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985nascp2358..136w&link_type=abstract

In NASA. Goddard Space Flight Center The Origin of Nonradiative Heating/Momentum in Hot Stars p 136-140 (SEE N85-17755 08-88)

Mathematics

Chaos, Hot Stars, Momentum Transfer, Particle Acceleration, Radio Emission, Stellar Winds, Synchrotron Radiation, Flow Stability, Mathematical Models, Prediction Analysis Techniques, Shock Waves

Scientific paper

A model is presented for the radio emission from hot stars. Electrons are accelerated to relativistic energies by shocks in the wind near the star and emit radio radiation through the synchrotron mechanism. The particle spectrum and radio spectrum for this model are derived. The model accounts for many of the observed characteristics of some recently discovered stars which have peculiar radio emission.

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