THERMAL AND DYNAMICAL BALANCE IN DENSE MOLECULAR CLOUD CORES

Citation
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
Citations number
34
Categorie Soggetti
Astronomy & Astrophysics
ISSN journal
00358711
Volume
288
Issue
3
Year of publication
1997
Pages
674 - 678
Database
ISI
SICI code
0035-8711(1997)288:3<674:TADBID>2.0.ZU;2-3
Abstract
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.