Grain temperatures in diffuse clouds and the depletion of interstellar argon

Details Grain temperatures in diffuse clouds and the depletion of interstellar argon Grain temperatures in diffuse clouds and the depletion of interstellar argon

Mar 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.190..683d&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 190, Mar. 1980, p. 683-687. Research supported by the Natural Sciences

Astronomy and Astrophysics

Astronomy

4

Argon, Granular Materials, Interstellar Gas, Interstellar Matter, Temperature Effects, Chemical Composition, Partial Pressure, Refractory Materials, Solid Surfaces

Scientific paper

The possible depletion of interstellar Ar and its relation to grain
temperature and grain composition in diffuse clouds is discussed. Ar
depletion is shown to require grain temperatures that are certainly less
than 36 K and very likely less than 20 K. Observations of Ar depletion
may provide a useful probe of grain temperature in diffuse clouds.

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