Kinematics and physics of emitting plasma around super-massive black holes

Details Kinematics and physics of emitting plasma around super-massive black holes Kinematics and physics of emitting plasma around super-massive black holes

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jphcs..63a2018p&link_type=abstract

Journal of Physics: Conference Series, Volume 63, Issue 1, pp. 012018 (2007).

Physics

Scientific paper

A group of galaxies emits strong permitted and forbidden lines from the central part where a massive black hole is supposed to be located. The cores of this type of galaxies, so called Active Galactic Nuclei (AGN) are known as a most powerful sources of radiation in the Universe. Here we discuss the emitting plasma conditions in emitting line regions of AGN as well as methods which are in usage to determine the physical properties of the emitting plasma around super massive black holes.

Affiliated with

Also associated with

No associations

Rating

Kinematics and physics of emitting plasma around super-massive black holes 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 Kinematics and physics of emitting plasma around super-massive black holes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Kinematics and physics of emitting plasma around super-massive black holes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1084208