The excitation mechanism of the interstellar 6.7 GHz methanol maser

Details The excitation mechanism of the interstellar 6.7 GHz methanol maser The excitation mechanism of the interstellar 6.7 GHz methanol maser

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997cha%26a..21..438l&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 21, Issue 4, p. 438-442.

Astronomy and Astrophysics

Astrophysics

Scientific paper

We notice that the second kind of astronomical methanol maser with strong emission always coexists at both 6.7 GHz and 12.2 GHz and in association with compact H II regions and we are led to propose a new excitation mechanism-maser amplification of the 6.7 GHz maser without population inversion. We show that this mechanism is compatible with the astronomical conditions and that it and other mechanisms are not mutually exclusive, rather it may serve as a useful complement.

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