Possibilities of observing dust in high-velocity H I clouds

Details Possibilities of observing dust in high-velocity H I clouds Possibilities of observing dust in high-velocity H I clouds

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993azh....70..649t&link_type=abstract

Astronomicheskij Zhurnal (ISSN 0004-6299), vol. 70, no. 3, p. 649-653.

Astronomy and Astrophysics

Astronomy

Cosmic Dust, Far Infrared Radiation, Hydrogen Clouds, Temperature Dependence, Milky Way Galaxy, Solar Radiation

Scientific paper

The possibility of detecting the presence of dust in high-velocity H I
clouds in the FIR is considered. Estimates of the brightness temperature
and surface brightness are made. The variation in dust temperature makes
it possible to independently estimate the distance to the high-velocity
clouds.

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