/ftp/cats/J_A+A/519//A27



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J/A+A/519/A27       CO maps in Serpens                    (Duarte-Cabral+, 2010)
The following files can be converted to FITS (extension .fit or fit.gz)
	maps.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/A+A/519/A27
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drwxr-xr-x 12 cats archive 215 Nov 5 2018 [Up] drwxr-xr-x 3 cats archive 269 Jan 12 2023 [TAR file] -rw-r--r-- 1 cats archive 466 Dec 19 2022 .message -r--r--r-- 1 cats archive 4099 Oct 3 2010 ReadMe -rw-r--r-- 1 cats archive 212 Oct 3 2010 +footg5.gif -rw-r--r-- 1 cats archive 2039 Oct 3 2010 +footg8.gif drwxr-xr-x 2 cats archive 100 Oct 3 2010 fig -r--r--r-- 1 cats archive 279 Jun 4 2010 maps.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+A/519/A27 CO maps in Serpens (Duarte-Cabral+, 2010) ================================================================================ The physical and dynamical structure of Serpens. Two very different sub-(proto) clusters. Duarte-Cabral A., Fuller G.A., Peretto N., Hatchell J., Ladd E.F., Buckle J., Richer J., Graves S.F. <Astron. Astrophys. 519, A27 (2010)> =2010A&A...519A..27D ================================================================================ ADC_Keywords: Radio sources ; Molecular clouds Keywords: stars: formation - ISM: kinematics and dynamics - ISM: molecules - ISM: clouds - ISM: structure Abstract: The Serpens North cluster is a nearby low mass star forming region which is part of the Gould belt. It contains a range of young stars thought to correspond to two different bursts of star formation and provides the opportunity to study different stages of cluster formation. This work aims to study the molecular gas in the Serpens North cluster to probe the origin of the most recent burst of star formation in Serpens. Transitions of the C^17^O and C^18^O observed with the IRAM 30m telescope and JCMT are used to study the mass and velocity structure of the region while the physical properties of the gas are derived using LTE and non-LTE analyses of the three lowest transitions of C^18^O. Description: cube_c17o_10.fits, cube_c18o_10.fits and cube_c18o_21.fits are the FITS files of the C^17^O(1-0), C^18^O(1-0) and C^18^O(2-1) raw data used in this paper, observed with the IRAM 30m telescope. Objects: ------------------------------------------------------- RA (2000) DE Designation(s) ------------------------------------------------------- 18 29 49 +01 14.8 Serpens = Name Serpens Cloud -------------------------------------------------------