/ftp/cats/aliases/G//GFM2007



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J/A+A/463/275   Chandra obs. of Serpens star-forming region    (Giardino+, 2007)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	table5.dat table6.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/A+A/463/275
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drwxr-xr-x 24 cats archive 4096 Jan 29 2012 [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 7778 Dec 1 2007 ReadMe -rw-r--r-- 1 cats archive 1009 Dec 1 2007 +footg5.gif -rw-r--r-- 1 cats archive 2949 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 7850 Oct 7 2007 table5.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 2314 Oct 7 2007 table6.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+A/463/275 Chandra obs. of Serpens star-forming region (Giardino+, 2007) ================================================================================ The onset of X-ray emission in young stellar objects. A Chandra observation of the Serpens star-forming region. Giardino G., Favata F., Micela G., Sciortino S., Winston E. <Astron. Astrophys., 463, 275-288 (2007)> =2007A&A...463..275G ================================================================================ ADC_Keywords: Associations, stellar ; YSOs ; Stars, pre-main sequence ; X-ray sources Keywords: ISM: clouds - ISM: individual objects: Serpens cloud - stars: pre-main sequence - X-rays: stars Abstract: To study the properties of X-ray emission from young stellar objects (YSOs) through their evolution from Class I to Class III and determine whether Class 0 protostars emit X-rays. A deep Chandra X-ray observation of the Serpens star-forming region was obtained. The Serpens Cloud Core is ideally suited for this type of investigation, being populated by a dense and extremely young cluster whose members are found in all evolutionary stages, including six well-studied Class 0 sources. Description: The core of the Serpens cloud was observed with Chandra starting at 21:43 UT on June 19, 2004. The observation lasted for 91.4ks (although the scheduled duration was 100ks).