Browsing by Subject "galaxies: Magellanic Clouds"
Now showing items 1-3 of 3
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(1988-08-15)A complete CO survey of the central 6 deg x 6 deg of the LMC was performed in order to determine the distribution of molecular clouds. At least 10 percent of the region studied exhibits CO line emission, with peak line ...
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(EDP Sciences, 2003-08)We present J = 1−0 and J = 2−1 12CO maps of several star-forming regions in both the Large and the Small Magellanic Cloud, and briefly discuss their structure. Many of the detected molecular clouds are relatively isolated ...
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(2002)We report observations of the CO(1!0), CO(2!1) and 13CO(1!0) line emission from the giant molecular complex No. 37 of the Large Magellanic Cloud, made with linear resolutions between 6 and 12 pc. The observations were ...