Galactic stellar orbits in the postepicyclic approximation

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Orbit Calculation, Stellar Motions, Stellar Orbits, Trajectory Analysis, Approximation, Density Wave Model, Epicycloids, Plasma Drift

Scientific paper

Relationships are found for the galactic orbits of stars in the second order of the epicyclic theory. An explicit expression is derived, describing the drift motion of stars along a circular trajectory in the rotating discs of galaxies. This small drift motion, which adds to the circular one, is analogous to the magnetic drift of plasma charged particles and is due to the differential rotation of the system. It is shown that, because of the stars' drift motion in the galactic disc's regions which are at the boundary of Jeans' stability, excitation is possible of gravitation-gradient instability of nonaxisymmetric perturbations of the gravitational potential and of the surface density. Due to its small increment, this gradient instability cannot serve as the mechanism generating global spiral density waves in the stellar disc of our Galaxy.

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

Galactic stellar orbits in the postepicyclic approximation 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 Galactic stellar orbits in the postepicyclic approximation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Galactic stellar orbits in the postepicyclic approximation will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-848285

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