Time dependent behavior of interstellar maser features due to stimulated scattering through dense plasma clouds

Details Time dependent behavior of interstellar maser features due to stimulated scattering through dense plasma clouds Time dependent behavior of interstellar maser features due to stimulated scattering through dense plasma clouds

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.251..325m&link_type=abstract

In ESA Proceedings of the Joint Varenna-Abastumani International School and Workshop on Plasma Astrophysics p 325-330 (SEE N87-

Astronomy and Astrophysics

Astrophysics

1

Compton Effect, Interstellar Masers, Plasma Clouds, Time Dependence, Backscattering, Radiant Flux Density, Water Masers

Scientific paper

Compact H2O interstellar sources of maser emission which show strong and rapid variability of flux intensity with time are discussed. It is suggested that stimulated ion-Compton or Brillouin backscattering of the superradiant radiation flux interacting with partially trapped radiation (due to reflection from the circumstellar plasma cloud boundaries), could explain such rapid time dependent behavior.

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