Astronomy and Astrophysics – Astronomy
Scientific paper
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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