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Issue A&A
Volume 453, Number 3, July III 2006
Page(s) 863 - 868
Section Extragalactic astronomy
DOI http://dx.doi.org/10.1051/0004-6361:20054664



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. Zhao1

1  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]$\lambda$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 $\mu$m) properties for a sample of 65 Seyfert 2 galaxies.
Methods.By using the AGN/Bulge/Disk decomposition technique, we analyzed the 2MASS $K_{\rm S}$-band images for Seyfert 2 galaxies in order to derive the $K_{\rm S}$-band magnitudes for the central engine, bulge, and disk components.
Results.We find that the $K_{\rm S}$-band magnitudes of the central AGN component in Seyfert 2 galaxies are tightly correlated with the [O III]$\lambda$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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