Brightness temperature and flux density of an astrophysical saturated maser

Details Brightness temperature and flux density of an astrophysical saturated maser Brightness temperature and flux density of an astrophysical saturated maser

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993phla..178...54w&link_type=abstract

Physics Letters A, Volume 178, Issue 1-2, p. 54-58.

Physics

2

Scientific paper

This Letter presents a more general formalism to derive a formula for the brightness temperature and flux density of an astrophysical saturated maser, showing that those predicted by the traditional theory are smaller, and also predicts that the two observable physical quantities increase with increasing elastic collision rate. This may help explain some important observed astrophysical maser phenomena.

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