/ftp/cats/aliases/M//MMS



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J/A+A/426/119  1.2mm mapping of RCW 106 Giant Molecular Cloud (Mookerjea+, 2004)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	table1.dat table2.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/A+A/426/119
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drwxr-xr-x 18 cats archive 321 Sep 27 2016 [Up] drwxr-xr-x 2 cats archive 288 Jan 13 2023 [TAR file] -rw-r--r-- 1 cats archive 482 Dec 19 2022 .message -r--r--r-- 1 cats archive 5313 Dec 5 2007 ReadMe -rw-r--r-- 1 cats archive 614 Dec 5 2007 +footg5.gif -rw-r--r-- 1 cats archive 2177 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 5510 Sep 9 2005 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 3143 Dec 4 2005 table2.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+A/426/119 1.2mm mapping of RCW 106 Giant Molecular Cloud (Mookerjea+, 2004) ================================================================================ The Giant Molecular Cloud associated with RCW 106. A 1.2 mm continuum mapping study. Mookerjea B., Kramer C., Nielbock M., Nyman L.-A. <Astron. Astrophys., 426, 119-129 (2004)> =2004A&A...426..119M ================================================================================ ADC_Keywords: H II regions ; Molecular clouds ; X-ray sources ; Radio sources; Infrared sources Keywords: ISM: clouds - ISM: dust, extinction - ISM: H II regions - ISM: structure - stars: formation - ISM: individual objects: RCW 106 Abstract: We have mapped the dust continuum emission from the molecular cloud covering a region of 28pcx94pc associated with the well-known H II region RCW 106 at 1.2mm using SIMBA on SEST. The observations, having an HPBW of 24" (0.4pc), reveal 95 clumps, of which about 50% have MSX associations and only 20% have IRAS associations. Owing to their higher sensitivity to colder dust and higher angular resolution the present observations identify new emission features and also show that most of the IRAS sources in this region consist of multiple dust emission peaks. The detected millimeter sources (MMS) include on one end the exotic MMS5 (associated with IRAS 16183-4958, one of the brightest infrared sources in our Galaxy) and the bright (and presumably cold) source MMS54, with no IRAS or MSX associations on the other end. Around 10% of the sources are associated with signposts of high mass star formation activity. Description: The 1.2mm continuum observations were carried out with the 37 channel bolometer array SIMBA (SEST Imaging Bolometer Array) at the SEST (Swedish-ESO Submillimeter Telescope) on La Silla, Chile during the night from July 4 to 5, 2002.