On heating by ion streams in H II/OH regions

Details On heating by ion streams in H II/OH regions On heating by ion streams in H II/OH regions

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....81..354e&link_type=abstract

Astronomy and Astrophysics, vol. 81, no. 3, Jan. 1980, p. 354, 355.

Astronomy and Astrophysics

Astrophysics

1

Hydrogen Clouds, Hydroxyl Emission, Interstellar Masers, Ionic Collisions, Radiant Cooling, Thermalization (Energy Absorption), Astrophysics, Carbon Monoxide

Scientific paper

Hartquist (1979) has argued recently that ion streams which could
invert H II/OH masers would also heat up the regions to unacceptably
high temperatures. I show that when cooling processes are analyzed
more carefully, the temperature in the maser region remains
sufficiently low in spite of the heating by ion friction.

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