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J/ApJ/703/736 Clump properties in the LMC 30 Dor region (Pineda+, 2009)
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Beginning of ReadMe :J/ApJ/703/736 Clump properties in the LMC 30 Dor region (Pineda+, 2009)
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The influence of far-ultraviolet radiation on the properties of molecular clouds
in the 30 Dor region of the Large Magellanic Cloud.
Pineda J.L., Ott J., Klein U., Wong T., Muller E., Hughes A.
<Astrophys. J., 703, 736-751 (2009)>
=2009ApJ...703..736P
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ADC_Keywords: Carbon monoxide ; Magellanic Clouds ; Molecular clouds ;
Interstellar medium ; Ultraviolet
Keywords: galaxies: ISM - ISM: molecules - ISM: structure - Magellanic Clouds
Abstract:
We present a complete ^12^CO(J=1-0) map of the prominent molecular
ridge in the Large Magellanic Cloud (LMC) obtained with the 22m ATNF
Mopra Telescope. The region stretches southward by 2deg (or 1.7kpc)
from 30 Doradus, the most vigorous star-forming region in the Local
Group. The location of this molecular ridge is unique insofar as it
allows us to study the properties of molecular gas as a function of
the ambient radiation field in a low-metallicity environment. The mass
spectrum and the scaling relations between the properties of the CO
clumps in the molecular ridge are similar, but not identical, to those
that have been established for Galactic molecular clouds.
Description:
The ^12^CO(J=1-0) (115GHz) observations were made using the 22m ATNF
Mopra Telescope between 2005 June and September. A total of 120
fields, 5'x5' in size, were mapped using the on-the-fly mapping mode,
encompassing the entire 30 Dor molecular ridge.