========================================================================== J/A+A/447/89 Luminous AGB stars in nearby galaxies (Tsalmantza+, 2006) The following files can be converted to FITS (extension .fit .fgz or .fiZ) smc.dat m31.dat m33.dat lmc.dat ========================================================================== Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/447/89 ==========================================================================
drwxr-xr-x 13 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 489 Jan 2 2007 .message -r--r--r-- 1 cats archive 2752 Jan 1 2007 ReadMe -rw-r--r-- 1 cats archive 670 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 2540 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 15768 Nov 25 2005 lmc.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 7300 Nov 25 2005 m31.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 2263 Nov 25 2005 m33.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 2482 Nov 25 2005 smc.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+A/447/89 Luminous AGB stars in nearby galaxies (Tsalmantza+, 2006) ================================================================================ Luminous AGB stars in nearby galaxies: A study using Virtual Observatory tools. Tsalmantza P., Kontizas E., Cambresy L., Genova F., Dapergolas A., Kontizas M. <Astron. Astrophys. 447, 89 (2006)> =2006A&A...447...89T ================================================================================ ADC_Keywords: Galaxies, nearby ; Stars, giant ; Photometry, infrared Keywords: stars: carbon - Local group - stars: AGB and post-AGB - infrared: stars - Magellanic Clouds Abstract: This study focuses on very luminous (M_bol_<-6.0mag) AGB stars with J-Ks>1.5mag and H-Ks>0.4mag in the LMC, SMC, M 31, and M 33 from 2MASS data. Description: The data were taken from the 2MASS All-Sky Point Source catalogue archive. We used Virtual Observatory tools and took advantage of its capabilities at various stages in the analysis.
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