Radiative shock models for the NLR of AGN: Predictions up to 1000 km s-1

Details Radiative shock models for the NLR of AGN: Predictions up to 1000 km s-1 Radiative shock models for the NLR of AGN: Predictions up to 1000 km s-1

Nov 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..222..305a&link_type=abstract

The Interplay among Black Holes, Stars and ISM in Galactic Nuclei, Proceedings of IAU Symposium, No. 222. Edited by T. Storchi-B

Computer Science

2

Scientific paper

High velocity shocks may provide an important source of ionizing radiation in the NLR of active galaxies. Here we present preliminary results of a new grid of MAPPINGS III shock models for shock velocities up to 1000 km s-1. This grid significantly extends the parameter space covered by the previous models, and will serve as an important component in building multi-process models of the NLR.

Affiliated with

Also associated with

No associations

Rating

Radiative shock models for the NLR of AGN: Predictions up to 1000 km s-1 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 Radiative shock models for the NLR of AGN: Predictions up to 1000 km s-1, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radiative shock models for the NLR of AGN: Predictions up to 1000 km s-1 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1112987