Nonlinear interaction of a spiral wave with stars near the corotation radius in disks of galaxies

Details Nonlinear interaction of a spiral wave with stars near the corotation radius in disks of galaxies Nonlinear interaction of a spiral wave with stars near the corotation radius in disks of galaxies

Feb 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980pazh....6...87m&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 6, Feb. 1980, p. 87-91.) Soviet Astronomy Letters, vol. 6, Jan.-Feb. 1980, p. 48-50. Tr

Astronomy and Astrophysics

Astronomy

Density Wave Model, Galactic Rotation, Spiral Galaxies, Star Distribution, Stellar Motions, Angular Momentum, Distribution Functions, Energy Transfer, Galactic Structure, Hamiltonian Functions, Momentum Transfer, Radii

Scientific paper

Nonlinear interaction of stars with a spiral gravitational-potential wave near the corotation radius will produce a plateau in the stellar distribution function after a few revolutions of the galaxy. This effect will terminate the resonance mechanism that builds up the spiral wave. The wave saturation level determined by the resonance mechanism is much smaller than the level observed.

Affiliated with

Also associated with

No associations

Rating

Nonlinear interaction of a spiral wave with stars near the corotation radius in disks of 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 Nonlinear interaction of a spiral wave with stars near the corotation radius in disks of galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Nonlinear interaction of a spiral wave with stars near the corotation radius in disks of galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1622312