Modeling the dynamical profile of a BL Lacertae object

Details Modeling the dynamical profile of a BL Lacertae object Modeling the dynamical profile of a BL Lacertae object

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008an....329..413p&link_type=abstract

Astronomische Nachrichten, Vol.329, Issue 4, p.413

Astronomy and Astrophysics

Astronomy

Galaxies: Kinematics And Dynamics

Scientific paper

A simple dynamical model for a BL Lacertae active galaxy is presented. The model consists of a logarithmic potential with an additional term representing internal perturbations. The time independent and the evolving model are investigated. In both cases we search for regular and chaotic motion and study the velocity distribution near the centre of the system. Numerical calculations suggest that responsible for the chaotic phenomena is the internal perturbation, the flattening parameter and the dense nucleus. The radius of the nucleus also affects the maximum velocity in the central regions of the galaxy. Our numerical outcomes are supported by theoretical arguments and analytical calculations. A linking of our numerical outcomes to observational data is also presented.

Affiliated with

Also associated with

No associations

Rating

Modeling the dynamical profile of a BL Lacertae object 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 Modeling the dynamical profile of a BL Lacertae object, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Modeling the dynamical profile of a BL Lacertae object will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1406469