Statistics – Computation
Scientific paper
Sep 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...360...30r&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 360, Sept. 1, 1990, p. 30-40. Research supported by Georgia State Universit
Statistics
Computation
5
Active Galactic Nuclei, Intergalactic Media, Radio Jets (Astronomy), Boundary Value Problems, Computational Astrophysics, Halos, Radio Galaxies, Red Shift
Scientific paper
Jets emanating from active galactic nuclei are simulated here by a boundary-following code as they propagate through a bimodal external medium consisting of an isothermal galactic halo and a hotter, less dense, uniform intergalactic medium (IGM). The maximum linear sizes of the beams are found as functions of the beam and media parameters, and some of the observed radio source size statistics are produced in a theoretical model which includes an IGM with a constant local density and temperature. Monte Carlo simulations are used to find the median distance for plausible distributions of various input parameters for a number of constant values of IGM density and temperature.
No associations
LandOfFree
Effect of an intergalactic medium on the average sizes of extragalactic jets 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 Effect of an intergalactic medium on the average sizes of extragalactic jets, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Effect of an intergalactic medium on the average sizes of extragalactic jets will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1400989