AAS Meeting #193 - Austin, Texas, January 1999
Session 6. Nearby AGN I - Dust, Gas, Obscuration and Fuelling
Display, Wednesday, January 6, 1999, 9:20am-6:30pm, Exhibit Hall 1
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[6.21] A Study of the Brightest Radio Emitting X-ray Galaxies
F. E. Bauer, J. J. Condon (National Radio Astronomy Observatory), T. X. Thuan (University of Virginia)
We present the results from a complete sample of galaxies
which are both radio sources in the 1.4 GHz NRAO VLA Sky
Survey (NVSS) and X-ray sources above 0.1 cnt/s in the ROSAT
All-Sky Survey Bright Source Catalog (BSC). This sample is
unique in its size (N\approx1500 galaxies and quasars),
composition (a mixture of nearly normal galaxies, Seyferts,
quasars, and clusters), and low average distance (
\approx0.1). We have obtained redshifts and classifications
for the majority of a magnitude-limited (J \leq 18 and
\delta \ge -20\deg) subsample. The spectra permit us to
estimate multivariate radio-X-ray-optical luminosity
functions of these local galaxies and model evolutionary
effects as a function of classification type. We use IRAS
data (detections and upper limits) to determine the dominant
energy source (AGN, stars and stellar remnants, or hot gas)
in most cases. Using optical spectra, IRAS luminosities or
limits, and high-resolution 4.5 & 8 GHz VLA data, we test
orientation-dependent "unified" models involving
relativistic beaming and absorption by nuclear dust torii.
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