Astronomy and Astrophysics – Astrophysics
Scientific paper
2000-01-26
Astrophys.Space Sci. 272 (2000) 189-196
Astronomy and Astrophysics
Astrophysics
to appear in: 1999, Proc. "Astrophysical Dynamics", eds. D. Berry et al., Astroph. Sp. Sci., in press
Scientific paper
10.1023/A:1002684126855
2d hydrodynamical simulations are performed to examine the evaporation and condensation processes of giant molecular clouds in the hot phase of the interstellar medium. The evolution of cold and dense clouds is calculated in the subsonic stream of a hot tenuous plasma. Our code includes self-gravity, heating and cooling processes and heat conduction by electrons. Significant differences occur between simulations with and without heat conduction.
Hensler Gerhard
Vieser Wolfgang
No associations
LandOfFree
Evaporation and Condensation Processes of Giant Molecular Clouds in a Hot Plasma does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Evaporation and Condensation Processes of Giant Molecular Clouds in a Hot Plasma, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evaporation and Condensation Processes of Giant Molecular Clouds in a Hot Plasma will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-54317