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A&A 453, 863-868 (2006)
DOI: 10.1051/0004-6361:20054664
The K-band properties of Seyfert 2 galaxies
Z. Peng1, Q. Gu1, J. Melnick2 and Y. Zhao11 Department of Astronomy, Nanjing University, Nanjing 210093, PR China
e-mail: [qsgu;yhzhao]@nju.edu.cn
2 European Southern Observatory, Alonso de Cordova 3107, Santiago, Chile
e-mail: jmelnick@eso.org
(Received 8 December 2005 / Accepted 15 March 2006)
Abstract
Aims. It is well known that the [O III]
5007 emission
line and hard X-ray (2-10 keV) luminosities are good indicators of
AGN activities and that the near and mid-infrared emission of
AGN originates from re-radiation of dusty clouds heated
by the UV/optical radiation from the accretion disk. In this paper
we present a study of the near-infrared K-band (2.2
m)
properties for a sample of 65 Seyfert 2 galaxies.
Methods.By using the AGN/Bulge/Disk decomposition technique, we analyzed
the 2MASS
-band images for Seyfert 2 galaxies in order
to derive the
-band magnitudes for the central engine,
bulge, and disk components.
Results.We find that the
-band magnitudes of the central
AGN component in Seyfert 2 galaxies are tightly correlated with
the [O III]
5007 and the hard X-ray luminosities,
which suggests that the AGN K-band emission is also an excellent
indicator of the nuclear activities at least for Seyfert 2
galaxies. We also confirm the good relation between the central
black hole masses and bulge's K-band magnitudes for Seyfert 2s.
Key words: galaxies: active -- galaxies: Seyfert -- infrared: galaxies -- methods: statistical
© ESO 2006
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