A model for the emission spectrum of active galactic nuclei

Details A model for the emission spectrum of active galactic nuclei A model for the emission spectrum of active galactic nuclei

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..93..277c&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 93, no. 2, June 1983, p. 277-280.

Astronomy and Astrophysics

Astrophysics

2

Active Galactic Nuclei, Astronomical Models, Emission Spectra, Intergalactic Media, Plasma Interactions, Galactic Radiation, Kinetic Energy, Magnetohydrodynamic Flow, Nonthermal Radiation, Plasma Heating, Shock Waves

Scientific paper

The overall spectrum of active galactic nuclei is discussed in terms of a wind and shock model. The central object of the active galactic nuclei is the source of a strong supercritical wind. The interaction of the wind with the surrounding medium generates the non-thermal radiation observed in active galactic nuclei. The spectrum predicted by the wind and shock model is compared with the observations of the quasar 3C 273.

Affiliated with

Also associated with

No associations

Rating

A model for the emission spectrum of active galactic nuclei 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 A model for the emission spectrum of active galactic nuclei, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A model for the emission spectrum of active galactic nuclei will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1504593