/ftp/cats/J/A%252BAS/117/261



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J/A+AS/117/261  BR photometry of galaxies in low density regions (Vennik+, 1996)
The following files can be converted to FITS (extension .fit .fit.Z .fgz)
	table5 table6 table7 table8
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/A+AS/117/261
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drwxr-xr-x 19 cats archive 332 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 266 Jan 12 2023 [TAR file] -rw-r--r-- 1 cats archive 488 Dec 19 2022 .message -r--r--r-- 1 cats archive 7205 Jun 17 1996 ReadMe -rw-r--r-- 1 cats archive 353 Mar 6 2013 +footg5.gif -rw-r--r-- 1 cats archive 2443 Mar 6 2013 +footg8.gif -r--r--r-- 1 cats archive 7075 Mar 26 1996 table5 -r--r--r-- 1 cats archive 738 Mar 26 1996 table6 -r--r--r-- 1 cats archive 6334 Mar 26 1996 table7 -r--r--r-- 1 cats archive 777 Mar 26 1996 table8
Beginning of ReadMe : J/A+AS/117/261 BR photometry of galaxies in low density regions (Vennik+, 1996) ================================================================================ Surface photometry of galaxies in low density regions. Vennik J., Hopp U., Kovachev B., Kuhn B., Elsaesser H. <Astron. Astrophys. Suppl. Ser. 117, 261 (1996)> =1996A&AS..117..261V (SIMBAD/NED BibCode) ================================================================================ ADC_Keywords: Photometry, surface Keywords: large scale structure of Universe - galaxies: photometry - fundamental parameters - structure Description: We perform detailed surface photometry, based on B- and/or R-band CCD images of 92 faint galaxies. They are a subsample of those galaxies which were studied by Hopp et al. (1994) in the direction of three nearby voids. We derive integral photometric parameters and radial surface brightness profiles and compare them to those of several faint galaxy samples, located in different environments, and of a bright field galaxy sample. According to the obtained photometric characteristics, our sample is a mixture of intrinsically bright and faint galaxies, about 60% of them belonging to the bright subsample (M_B_<-19.0). These bright ones show mean characteristics of typical Freeman's disks and are mainly located in the background of the observed voids. The faint subsample (M_B_>=-19.0) has parameters typical for the low-surface-brightness (LSB) galaxies. There are a few well isolated galaxies both among the bright and faint subsamples.