Composite models for the narrow line region of galactic nuclei. IV - The intermediate Seyfert galaxies

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

20

Astronomical Models, Galactic Nuclei, Seyfert Galaxies, Spectral Line Width, Spectrum Analysis, Active Galactic Nuclei, Astronomical Spectroscopy, Emission Spectra, Photoionization, Shock Waves

Scientific paper

In this paper the analysis of the emission line spectra of Seyfert galaxies is continued in the light of the composite models for the narrow line region of active galactic nuclei. The model accounts for the coupled effect of photoionization and shock waves in determining the physical conditions in the emitting clouds. Therefore, some calculations about densities and temperatures in the postshock region are presented in the range of the observed values, and correlations with shock velocities are discussed. The observed data of a particular group of galaxies, called intermediate Seyfert galaxies (Cohen, 1983) are compared to model calculations. From the point of view of narrow lines, the results show that Seyfert type 2, intermediate Seyfert galaxies, and Liners may be interpreted as different aspects of the same phenomenon, depending only on the relative importance of photoionization and shock effects in determining the physical conditions of the emitting region.

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

Composite models for the narrow line region of galactic nuclei. IV - The intermediate 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 Composite models for the narrow line region of galactic nuclei. IV - The intermediate Seyfert galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Composite models for the narrow line region of galactic nuclei. IV - The intermediate Seyfert galaxies will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1147403

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