CO and IRAS detection of an intermediate-velocity cloud

Details CO and IRAS detection of an intermediate-velocity cloud CO and IRAS detection of an intermediate-velocity cloud

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...355l..51d&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 355, June 1, 1990, p. L51-L54.

Astronomy and Astrophysics

Astronomy

19

Carbon Monoxide, Molecular Clouds, Cosmic Dust, Emission, Infrared Astronomy Satellite, Interstellar Matter

Scientific paper

In the course of a radio survey of high-Galactic-latitude clouds, CO emission was detected at the position l = 210.8 deg and b = 63.1 deg with an LSR velocity of -39 km/sec. This molecular cloud constitutes the third one with an unusually large absolute velocity at these latitudes, as compared with the 5.4-km/sec cloud-to-cloud velocity dispersion of the high-latitude molecular clouds. The position is coincident with an H I intermediate-velocity cloud (GHL 11, Verschuur H, OLM 268) and the IR-excess cloud 306 in the list by Desert et al. (1988). This cloud is clearly detected at all four IRAS wavelengths and has warmer colors than the local ISM.

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