========================================================================== J/ApJ/542/673 Morphological types of galaxies in clusters (Fasano+, 2000) The following files can be converted to FITS (extension .fit .fgz or .fiZ) table2.dat table3.dat table5.dat ========================================================================== Query from: http://vizier.u-strasbg.fr/cgi-bin/VizieR?-source=J/ApJ/542/673 ==========================================================================
drwxr-xr-x 4 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 May 12 10:01 [TAR file] -rw-r--r-- 1 cats archive 489 Mar 31 2001 .message -r--r--r-- 1 cats archive 6351 Mar 31 2001 ReadMe -rw-r--r-- 1 cats archive 670 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 2719 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 331 Mar 26 2001 table2.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 4433 Mar 26 2001 table3.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 322 Mar 19 2001 table5.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/ApJ/542/673 Morphological types of galaxies in clusters (Fasano+, 2000) ================================================================================ The evolution of the galactic morphological types in clusters. Fasano G., Poggianti B.M., Couch W.J., Bettoni D., Kjaergaard P., Moles M. <Astrophys. J. 542, 673 (2000)> =2000ApJ...542..673F ================================================================================ ADC_Keywords: Clusters, galaxy ; Morphology ; Redshifts Keywords: galaxies: clusters: general - galaxies: evolution - galaxies: structure Abstract: The morphological types of galaxies in nine clusters in the redshift range 0.1< z< 0.25 are derived from very good seeing images taken at the North Optical Telescope (NOT) and the La Silla-Danish telescopes, with all galaxies at M_V_<-20 and within the central 1Mpc^2^ area being classified. With the purpose of investigating the evolution of the fraction of different morphological types with redshift, we compare our results with the morphological content of nine distant clusters studied by the MORPHS group, five clusters observed with HST/WFPC2 at redshift z=0.2-0.3, and Dressler's large sample of nearby clusters.
© UDS/CNRS