OH main line masers. II - H II/OH regions

Details OH main line masers. II - H II/OH regions OH main line masers. II - H II/OH regions

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....73..322e&link_type=abstract

Astronomy and Astrophysics, vol. 73, no. 3, Mar. 1979, p. 322-328.

Astronomy and Astrophysics

Astrophysics

20

Hydroxyl Emission, Interstellar Masers, Line Spectra, Magnetic Pumping, Population Inversion, H Ii Regions, Interstellar Magnetic Fields, Magnetic Field Configurations, Particle Collisions

Scientific paper

The role of magnetic field and possible inversion mechanisms in OH main
line masers associated with compact H II regions (H II/OH regions, for
brevity) are discussed. It is argued that the most plausible explanation
for the inversion effect is collisions with particle streams, though the
exact nature of the pump is not established.

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