An explicit model for the different morphological types of galaxies

Details An explicit model for the different morphological types of galaxies An explicit model for the different morphological types of galaxies

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..81..387l&link_type=abstract

Astrophysics and Space Science, vol. 81, no. 1-2, Jan. 1982, p. 387-395. In French.

Astronomy and Astrophysics

Astrophysics

Astronomical Models, Density Wave Model, Galactic Structure, Poisson Equation, Boltzmann Transport Equation, Spiral Galaxies

Scientific paper

In the now classical Lindblad-Lin density-wave theory, the linearization of the collisionless Boltzmann equation is made by assuming the potential function U expressed in the form U U0 + U + Where U0 is the background axisymmetric potential and U ~ U0. Then the corresponding density distribu- tion is p Po + j5(j~ ~ Po) and the linearized equation connecting U and the component f of the distribution function is given b

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