==========================================================================
J/other/PBeiO/18.7 Far infrared Seyfert galaxies (Liu 1991)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
table1 table2 table3 table4
==========================================================================
Query from: http://vizier.cds.unistra.fr/cgi-bin/VizieR?-source=J/other/PBeiO/18.7
==========================================================================
drwxr-xr-x 8 cats archive 151 Mar 16 2012 [Up]
drwxr-xr-x 2 cats archive 323 Jan 13 2023 [TAR file]
-rw-r--r-- 1 cats archive 480 Dec 19 2022 .message
-r--r--r-- 1 cats archive 2986 Oct 31 1997 ReadMe
-rw-r--r-- 1 cats archive 213 Sep 19 2007 +footg5.gif
-rw-r--r-- 1 cats archive 2047 Mar 5 2008 +footg8.gif
-r--r--r-- 1 cats archive 2975 Jun 3 1994 table1
-rw-r--r-- 1 cats archive 6035 Feb 24 1998 table2
-r--r--r-- 1 cats archive 1020 Jun 1 1994 table3
-r--r--r-- 1 cats archive 1360 Jun 1 1994 table4 Beginning of ReadMe :J/other/PBeiO/18.7 Far infrared Seyfert galaxies (Liu 1991)
================================================================================
Far infrared Seyfert galaxies and their confusing point sources
Liu Y.-L.
<Publ. Beijing Astron. Obs., 18, 7 (1991)>
=1991PBeiO..18....7L
================================================================================
ADC_Keywords: Galaxies, Seyfert ; Galaxies, IR
Description:
Confusing sources of Seyfert and HII galaxies in IRAS point source
catalogue may be caused by companion objects of those galaxies.
Comparison between confused galaxies and non-confused galaxies
have been made. The preliminary comparison shows that confused
galaxies are fainter than nonconfused galaxies generally, and
colour diagrams illustrate that confused Seyferts are separated
from nonconfused Seyferts obviously.