The cold interstellar gas and the stability of galactic discs.

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

The author has made use of simplified models of galactic discs in which the stars and the cold interstellar gas are treated as two different components. Although such models might be thought of as being inaccurate to describe actual galactic discs, which are known to consist of different populations of stars and gas components, they incorporate indeed the most essential features as regard their stability properties. It is found that the stabilizing role of finite-thickness effects can partially counterbalance the destabilizing role of the cold interstellar gas in linear regimes.

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