Multi-component Spectral Energy Distribution Fitting of Nearby SeyfertGalaxies

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

We present multi-component spectral energy distribution fitting of a sample of nearby Seyfert galaxies observed by the Infrared Spectrograph on the Spitzer Space Telescope between 5 and 35 μm. The sample was selected to represent a wide range of x-ray determined column densities and so, within the context of the unified model, covers a large number of possible viewing angles to the cores of the active galactic nuclei. The fits separate the SEDs into continuum emission from graphite and silicate grains at different characteristic temperatures, feature emission from PAH molecules, and atomic and molecular line emission.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Multi-component Spectral Energy Distribution Fitting of Nearby SeyfertGalaxies 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 Multi-component Spectral Energy Distribution Fitting of Nearby SeyfertGalaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Multi-component Spectral Energy Distribution Fitting of Nearby SeyfertGalaxies will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1395582

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.