The relationship between the cold and dense regions in Rho OPH: The DCOT lines

Details The relationship between the cold and dense regions in Rho OPH: The DCOT lines The relationship between the cold and dense regions in Rho OPH: The DCOT lines

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982esasp.192...93l&link_type=abstract

In ESA Galactic and Extragalactic Infrared Spectroscopy p 93-99 (SEE N83-18593 08-88)

Physics

6

Emission Spectra, Molecular Clouds, Star Clusters, Supernova Remnants, Zodiacal Dust, Atmospheric Attenuation, Carbon Dioxide, Hydrogen, Magnetic Fields, Mass, Shock Layers, Stellar Evolution

Scientific paper

The four lowest DCO(+) transitions have been observed in a region of the Rho Oph cloud. The unusually strong DCO(+) emission requires the presence of a very dense and cold molecular cloud core. Adjacent to this DCO(+) emission core is a region of rare 2 cm H2CO emission which is interpreted as a shocked layer propagating into the DCO(+) region. This shock arises from the interaction of an old supernova remnant and the molecular cloud.

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