The dependence of interstellar element depletions on mean space density

Details The dependence of interstellar element depletions on mean space density The dependence of interstellar element depletions on mean space density

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984nascp2349..204h&link_type=abstract

In NASA. Goddard Space Flight Center Future of Ultraviolet Astronomy Based on Six Years of IUE Res. p 204-206 (SEE N85-20961 1

Astronomy and Astrophysics

Astronomy

Depletion, Interstellar Chemistry, Interstellar Gas, Space Density, Chlorine, Iue, Oao 3, Ultraviolet Astronomy, Zinc

Scientific paper

Correlations of interstellar gas-phase depletions with hydrogen column density N(H), and with mean line-of-sight space density bar-n(H) = N(H)/r, are investigated for 14 elements. For the 6 most depleted elements, correlations ith bar-n(H) are clearly stronger than with N(H). In general, the survey supports the proposal that depletion is mainly governed by density-dependent processes. It also suggests that depletion occurs in relatively low density gas as well as in dense clouds.

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