J/A+A/298/375                       Jet-disk symbiosis II  (Falcke+ 1995)
The following files can be converted to FITS (extension .fit .fit.Z .fgz)
	table1 table2
Query from: http://vizier.u-strasbg.fr/cgi-bin/VizieR?-source=J/A+A/298/375

drwxr-xr-x 5 cats archive 105 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 Dec 15 09:37 [TAR file] -rw-r--r-- 1 cats archive 464 Feb 26 1999 .message -r--r--r-- 1 cats archive 5743 Jan 23 1999 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 11566 Jun 16 1995 table1 -r--r--r-- 1 cats archive 2005 Jun 16 1995 table2
Beginning of ReadMe : J/A+A/298/375 Jet-disk symbiosis II (Falcke+ 1995) ================================================================================ The jet-disk symbiosis II. Interpreting the Radio/UV correlations in quasars FALCKE H., MALKAN M.A., BIERMANN P.L. <Astron. Astrophys. 298, 375 (1995)> =1995A&A...298..375F (SIMBAD/NED Reference) ================================================================================ ADC_Keywords: QSOs; Galaxies, radio; Keywords: galaxies: active - galaxies: jets - galaxies: nuclei - accretion disks Description: We investigate the correlation between the accretion disk (UV) luminosity and the radio core emission of a quasar sample, containing all PG quasars, also deriving empirical conversion factors from emission line luminosities to disk luminosities. This method allows us to investigate the radio properties of AGN on the absolute scale set by the accretion power. The tables contain the quasar (and radio galaxy) sample discussed in this paper (including the complete PG quasars sample) and give the derived `disk luminosities' of the UV-bump and 5GHz radio luminosities.