Depletions and extinction curves for lines of sight through the outer edges of truly dense molecular clouds

Details Depletions and extinction curves for lines of sight through the outer edges of truly dense molecular clouds Depletions and extinction curves for lines of sight through the outer edges of truly dense molecular clouds

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986inpr.conf..135j&link_type=abstract

In NASA. Ames Research Center Summer School on Interstellar Processes: Abstracts of Contributed Papers p 135-136 (SEE N87-15043

Computer Science

Dust, Far Ultraviolet Radiation, Interstellar Extinction, Molecular Clouds, Abundance, Gas-Solid Interactions, Grain Size, Line Spectra, Size Distribution, Spectral Resolution

Scientific paper

Observations of a few moderately reddened (0.3 is less than E(B-V) is less than 0.6) lines of sight through the outer edges of truly dense molecular clouds, not only show the overall depletions in these clouds to be as much as 0.5 (dex) greater than in comparably reddened diffuse clouds, but reveal a possible tendency for certain species to deplete preferentially. Possible methods of depletions are discussed.

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