Relationship of groups of submillimeter starless condensations to radial systems of dark globules

Details Relationship of groups of submillimeter starless condensations to radial systems of dark globules Relationship of groups of submillimeter starless condensations to radial systems of dark globules

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ap.....53..112g&link_type=abstract

Astrophysics, Volume 53, Issue 1, pp.112-122

Astronomy and Astrophysics

Astrophysics

Dark Globules, Radial Systems, Submillimeter Starless Condensations

Scientific paper

The recently discovered groups of submillimeter starless condensations at the junction of HII regions and molecular clouds, which are invisible in the optical and near IR ranges, are similar in many ways to visible radial systems of dark globules, specifically, in their densities of molecular hydrogen, sizes, proximity to bright stars of early classes (which may be responsible for their formation), etc. It is proposed that the groups of submm starless condensations are radial systems of dark globules that are optically invisible because they lie behind dark clouds. Thus, it is shown that these groups of condensations are not a new type of object.

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