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Multi-Band Bar/Bulge/Disk Image Decomposition of a Thousand Galaxies

Published online by Cambridge University Press:  01 December 2006

Dimitri Gadotti  and
Guinevere Kauffmann
Dimitri Gadotti
Affiliation:
Max-Planck-Institut für Astrophysik Karl-Schwarzschild-Str. 1, D-85741, Garching bei München, Germany email: [email protected], [email protected]
Guinevere Kauffmann
Affiliation:
Max-Planck-Institut für Astrophysik Karl-Schwarzschild-Str. 1, D-85741, Garching bei München, Germany email: [email protected], [email protected]
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Abstract

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The structural parameters of bulges, disks and bars of a sample of nearly 1000 nearby galaxies are being determined through sophisticated image decomposition in the g, r and i bands. The sample is carefully drawn from the Sloan Digital Sky Survey Data Release 2 (SDSS DR2), contains 963 galaxies, of which 407 host AGN, and we show that it is representative of the galaxy and AGN populations in the local universe. A large number of other physical properties have also been determined for these galaxies within the SDSS collaboration. With these data, we reinforce several recent studies and find a number of results leading to new insights into how the different galaxy components relate to each other and the extent to which the hosts galaxies of AGN differ from quiescent galaxies.

Keywords

galaxies: activegalaxies: photometrygalaxies: structure
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S241: Stellar Populations as Building Blocks of Galaxies , December 2006 , pp. 507 - 508
Copyright
Copyright © International Astronomical Union 2007

References

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Heckman, T. et al. 2004, ApJ 613, 109CrossRefGoogle Scholar
Kauffmann, G. et al. 2006, ApJS in press (astro-ph/0609436)Google Scholar
Thomas, D. & Davies, R. 2006, MNRAS 366, 510CrossRefGoogle Scholar