Morphology and Photometry of Isolated Seyfert Galaxies

Details Morphology and Photometry of Isolated Seyfert Galaxies Morphology and Photometry of Isolated Seyfert Galaxies

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..396...55c&link_type=abstract

Formation and Evolution of Galaxy Disks ASP Conference Series, Vol. 396, Proceedings of the conference held 1-5 October, 2007 at

Mathematics

Logic

Scientific paper

An unresolved and intriguing problem about active galactic nuclei is the mechanism responsible for nuclear triggering and fueling. Until now there is not a unique solution that can completely explain this phenomenon. We present preliminary results about morphological and photometric analysis of a sample of 35 nearby (z<0.035) and isolated Seyfert galaxies, observed through broad-band BVR filters at the 1.8-m Vatican Telescope and the 2.2-m ESO-La Silla Telescope. We analyzed photometric and morphological parameters and, using GALFIT software, we obtained two-dimensional decomposition of the luminosity profiles.

Affiliated with

Also associated with

No associations

Rating

Morphology and Photometry of Isolated Seyfert Galaxies does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Morphology and Photometry of Isolated Seyfert Galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Morphology and Photometry of Isolated Seyfert Galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-771996