/ftp/cats/J/A+A/390/501



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J/A+A/390/501   Millimetre observations of carbon stars. I. (Groenewegen+, 2002)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	table1.dat table3.dat
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Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/390/501
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drwxr-xr-x 19 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 May 12 09:58 [TAR file] -rw-r--r-- 1 cats archive 480 Nov 13 2012 .message -r--r--r-- 1 cats archive 4668 Aug 22 2002 ReadMe -rw-r--r-- 1 cats archive 448 Nov 13 2012 +footg5.gif -rw-r--r-- 1 cats archive 4307 Nov 13 2012 +footg8.gif -r--r--r-- 1 cats archive 4272 Aug 22 2002 table1.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 8781 Aug 22 2002 table3.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+A/390/501 Millimetre observations of carbon stars. I. (Groenewegen+, 2002) ================================================================================ Millimetre Observations of Infrared Carbon Stars I: The Data Groenewegen M.A.T., Sevenster M., Spoon H.W.W., Perez I. <Astron. Astrophys. 390, 501 (2002)> =2002A&A...390..501G ================================================================================ ADC_Keywords: Stars, carbon ; Infrared sources ; Radio lines ; Radial velocities Keywords: circumstellar matter - stars: mass loss - stars: AGB and post-AGB - radio lines: stars Abstract: Millimetre observations of IRAS selected red carbon stars are presented. About 260 stars have been observed with SEST and IRAM in the CO (1-0) and CO (2-1) lines and partially in HCN (1-0) and SiO (3-2). An overall detection rate, in at least one line, of about 80% is achieved. The survey represents the second largest survey for AGB stars, and the largest ever for carbon stars. Two new detections in SiO (3-2) in carbon stars are reported. When available, the SiO/HCN and HCN/CO(1-0) line ratios are consistent with the ratios expected for carbon stars. Description: The results of a large millimetre survey of infrared carbon stars is presented. The Table provides the detailed outcome of the observations. IRAS name, transition and molecule, velocity resolution, rms noise, peak temperature, integrated intensity, central velocity and expansion velocity are presented.

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