Precession in Extragalactic Parsec-Scale Accretion Disks

Details Precession in Extragalactic Parsec-Scale Accretion Disks Precession in Extragalactic Parsec-Scale Accretion Disks

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010iaus..267..325c&link_type=abstract

Co-Evolution of Central Black Holes and Galaxies, Proceedings of the International Astronomical Union, IAU Symposium, Volume 267

Astronomy and Astrophysics

Astronomy

1

Galaxies: Active, Accretion, Accretion Disks

Scientific paper

In this work, we study the feasibility of four physical mechanisms for driving jet/disk precession in the galaxies NGC 4258, NGC 1068, 3C 120, OJ 287 and Arp 102B. Given the many observational uncertainties that still exist in the parameters of those AGN, we find that it is difficult to discriminate unambiguously what mechanism is actually responsible for precession.

Affiliated with

Also associated with

No associations

Rating

Precession in Extragalactic Parsec-Scale Accretion Disks 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 Precession in Extragalactic Parsec-Scale Accretion Disks, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Precession in Extragalactic Parsec-Scale Accretion Disks will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-793611