Global instability of thin stellar discs

Details Global instability of thin stellar discs Global instability of thin stellar discs

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.119..199f&link_type=abstract

(IAU, Asian-Pacific Regional Meeting, 3rd, Kyoto, Japan, Sept. 30-Oct. 5, 1984) Astrophysics and Space Science (ISSN 0004-640X),

Astronomy and Astrophysics

Astrophysics

2

Boltzmann Distribution, Density Distribution, Stellar Structure, Systems Stability, Distribution Functions, Numerical Integration

Scientific paper

The authors have determined the dominant global modes of stellar discs
by integrating the linearized collisionless Boltzmann equation. The
models examined are the Kuzmin discs with two types of the distribution
function. It is found that the growth rate correlates well with the
central value of Q.

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