The determination of cloud masses and dust characteristics from submillimetre thermal emission

Details The determination of cloud masses and dust characteristics from submillimetre thermal emission The determination of cloud masses and dust characteristics from submillimetre thermal emission

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983stin...8324436h&link_type=abstract

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Physics

Clouds, Dust, Interstellar Matter, Mass, Thermal Emission, Emissivity, Far Infrared Radiation, Permittivity, Polarized Radiation, Submillimeter Waves

Scientific paper

The principles by which the dust and masses and total masses of
interstellar clouds and certain characteristics of interstellar dust
grains can be derived from observations of far infrared and
submillimeter thermal emission are reviewed. To the extent possible, the
discussion will be independent of particular grain models.

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