H I and dust in the high latitude dark cloud L 1642.

Details H I and dust in the high latitude dark cloud L 1642. H I and dust in the high latitude dark cloud L 1642.

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989iaus..135p.203l&link_type=abstract

IAU Symposium No. 135: Interstellar dust: contributed papers, p. 203 - 204

Physics

Dark Clouds: H I Regions, Dark Clouds: Dust Grains

Scientific paper

The authors have mapped the high latitude dark cloud L 1642 in the 21-cm H I line using the 100-m radio telescope at Effelsberg. A remarkable H I line broadening from 2.5 to 2.9 km/s is observed over a small area on the "bright side" of L 1642, i.e. the side facing the galactic plane. Results are presented concerning the effects of the asymmetrical UV radiation field of OB stars on the H I gas and the very small dust grains associated with L 1642.

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