Jeans instability of interstellar gas clouds in the background of weakly interacting massive particles

Details Jeans instability of interstellar gas clouds in the background of weakly interacting massive particles Jeans instability of interstellar gas clouds in the background of weakly interacting massive particles

1998-05-20

arxiv.org/abs/astro-ph/9805271v2

Astrophys.J. 507 (1998) 226-228

Astronomy and Astrophysics

Astrophysics

version accepted in ApJ, Nov. 1, 1998 issue, vol. 507

Scientific paper

10.1086/306334

Criterion of the Jeans instability of interstellar gas clouds which are
gravitationally coupled with weakly interacting massive particles is revisited.
It is established that presence of the dark matter always reduces the Jeans
length, and in turn, Jeans mass of the interstellar gas clouds. Astrophysical
implications of this effect are discussed.

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