On the extragalactic interpretation of high-velocity H I clouds

Details On the extragalactic interpretation of high-velocity H I clouds On the extragalactic interpretation of high-velocity H I clouds

Sep 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...208..694e&link_type=abstract

Astrophysical Journal, vol. 208, Sept. 15, 1976, pt. 1, p. 694-700.

Astronomy and Astrophysics

Astronomy

16

Extragalactic Radio Sources, Hydrogen Clouds, Interstellar Gas, Radio Astronomy, Electron Energy, Gas Cooling, High Speed, Hydrogen Atoms, Thermal Energy, Ultrahigh Frequencies

Scientific paper

The cooling rates of high-velocity H I clouds are examined under the hypothesis that such clouds are at distances on the order of a megaparsec. It is found that many of these clouds require support mechanisms other than stock thermal energy to sustain them at their present parameters. Support mechanisms, their plausibility, and their possible observational consequences are discussed.

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