Galaxy interactions have been suggested to play an important role in triggering AGN activity. In this context we have started to analyze morphological properties of nearby AGNs (z<0.1) and their environment. We have chosen an unbiased statistical complete flux-limited AGN sample of 101 Seyfert galaxies from the ROSAT Bright Survey (RBS). Here we present the research project and show first results.

Morphological analysis of a statistically complete x-ray selected sample of Seyfert galaxies

RAFANELLI, PIERO
2001

Abstract

Galaxy interactions have been suggested to play an important role in triggering AGN activity. In this context we have started to analyze morphological properties of nearby AGNs (z<0.1) and their environment. We have chosen an unbiased statistical complete flux-limited AGN sample of 101 Seyfert galaxies from the ROSAT Bright Survey (RBS). Here we present the research project and show first results.
2001
X-RAY ASTRONOMY: Stellar Endpoints,AGN, and the Diffuse X-ray Background
0735400431
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11577/1364587
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