Cj. Clarke et Je. Pringle, THERMAL AND DYNAMICAL BALANCE IN DENSE MOLECULAR CLOUD CORES, Monthly Notices of the Royal Astronomical Society, 288(3), 1997, pp. 674-678
We consider the thermal and dynamical balance in dense molecular cloud
cores. We point out that because such cores are heated throughout the
ir volumes by cosmic rays, but cool radiatively by means of optically
thick lines, they are likely to be dynamically unstable and at best in
only a form of quasi-static equilibrium. We also draw attention to th
e possibility that if such cores undergo an external impulse that s la
rge enough to produce a velocity difference Delta upsilon less than or
similar to c(s), where c(s) is the thermal sound speed, then the cool
ing rate rises suddenly and pressure support drops, which leads to gra
vitational collapse and fragmentation.