/ftp/cats/aliases/M/./MAGMA



==========================================================================
J/ApJS/197/16      The Magellanic Mopra Assessment (MAGMA). I.     (Wong+, 2011)
The following files can be converted to FITS (extension .fit or fit.gz)
	table[456].dat
==========================================================================
Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/ApJS/197/16
==========================================================================

drwxr-xr-x 16 cats archive 260 Feb 13 2012 [Up] drwxr-xr-x 2 cats archive 323 Jan 13 2023 [TAR file] -rw-r--r-- 1 cats archive 472 Dec 19 2022 .message -r--r--r-- 1 cats archive 5565 Feb 19 2012 ReadMe -rw-r--r-- 1 cats archive 1016 Mar 1 2021 +footg5.gif -rw-r--r-- 1 cats archive 2482 Mar 1 2021 +footg8.gif -r--r--r-- 1 cats archive 58764 Feb 19 2012 table4.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 62988 Feb 19 2012 table5.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 83744 Feb 19 2012 table6.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/ApJS/197/16 CO observations of LMC molecular clouds (MAGMA). (Wong+, 2011) ================================================================================ The Magellanic Mopra Assessment (MAGMA). I. The molecular cloud population of the Large Magellanic Cloud. Wong T., Hughes A., Ott J., Muller E., Pineda J.L., Bernard J.-P., Chu Y.-H., Fukui Y., Gruendl R.A., Henkel C., Kawamura A., Klein U., Looney L.W., Maddison S., Mizuno Y., Paradis D., Seale J., Daniel E.W. <Astrophys. J. Suppl. Ser., 197, 16 (2011)> =2011ApJS..197...16W ================================================================================ ADC_Keywords: Magellanic Clouds ; Molecular clouds ; Radial velocities ; Interstellar medium ; Radio lines ; Cross identifications Keywords: galaxies: ISM - ISM: molecules - Magellanic Clouds - stars: formation Abstract: We present the properties of an extensive sample of molecular clouds in the Large Magellanic Cloud (LMC) mapped at 11pc resolution in the CO(1-0) line. Targets were chosen based on a limiting CO flux and peak brightness as measured by the NANTEN survey. The observations were conducted with the ATNF Mopra Telescope as part of the Magellanic Mopra Assessment. We identify clouds as regions of connected CO emission and find that the distributions of cloud sizes, fluxes, and masses are sensitive to the choice of decomposition parameters. Description: Observations were performed with the Australia Telescope National Facility (ATNF) Mopra 22m telescope from 2005 May to 2010 October.