Molecules, grains, and shocks: a comparison of CO, H I and IRAS data.

Details Molecules, grains, and shocks: a comparison of CO, H I and IRAS data. Molecules, grains, and shocks: a comparison of CO, H I and IRAS data.

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989iaus..135p.301h&link_type=abstract

IAU Symposium No. 135: Interstellar dust: contributed papers, p. 301

Computer Science

Interstellar Clouds: Kinematics

Scientific paper

The authors have compared the IR and H I properties, and CO content, of
a set of 26 isolated, degree-sized interstellar clouds. The comparisons
offer some conclusions concerning the effects of kinematics on molecular
content and grain size distribution, although these conclusions are
provisional because of the small sample.

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