(C-18)O in the Chamaeleon I dark cloud

Details (C-18)O in the Chamaeleon I dark cloud (C-18)O in the Chamaeleon I dark cloud

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.171..219t&link_type=abstract

(IAU, European Regional Astronomy Meeting, 11th, La Laguna, Spain, July 3-8, 1989) Astrophysics and Space Science (ISSN 0004-640

Astronomy and Astrophysics

Astronomy

4

Carbon Monoxide, Dark Matter, Oxygen 18, Star Formation, Infrared Astronomy, Molecular Clouds, Stellar Mass, Telescopes

Scientific paper

The Epsilon Cha I dark cloud is nearby (140 pc) site of low-mass star formation. Due to its high Galactic latitude it is an observationally favorable object for study at radio as well as other wavelengths. The central part of the cloud has been mapped in the (C-18)O (1-0) line using both the 1.2-m Columbia Southern Millimeter-Wave Telescope at Cerro Tololo and the 15-m Swedish-ESO Submillimeter Telescope (SEST).

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