Stellar and gaseous dynamics of triaxial galaxies

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

47

Galactic Structure, Interstellar Gas, Stellar Motions, Active Galaxies, Elliptical Orbits, Galactic Rotation, Galerkin Method, Gas Dynamics, Hamiltonian Functions, Orbital Mechanics, Orbital Resonances (Celestial Mechanics)

Scientific paper

A variety of analytic means for examining the existence and stability of orbit families in triaxial potentials which approximate the potential fields of triaxial galaxies are presented. A particular class of potentials which possess three exact integrals of motion is analyzed. This potential is chosen because of its resemblance to the potential used by Schwarzschild (1979) to produce an equilibrium model of a triaxial stellar figure. The properties of a potential based on an expansion about the core region is explored, including the potential and the resulting integrals of motion for the 1-1-1 resonance and the stability of periodic orbits. The Galerkin method is used to solve for the resonant orbits to first order. New features of the central regions of galaxies are discussed, particularly the possibility of the formation of stable equilibrium tilted disks, the structure of the Spindle galaxy, and implications for enhanced fueling of gas into the central engine of active galaxies.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Stellar and gaseous dynamics of triaxial galaxies 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 Stellar and gaseous dynamics of triaxial galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stellar and gaseous dynamics of triaxial galaxies will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1626967

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.