Star formation through thermal instability of radiative plasma with finite electron inertia and finite Larmor radius corrections
I have studied the effects of finite electron inertia, finite ion Larmor radius (FLR) corrections, and radiative heat-loss function on the thermal instability of an infinite homogeneous, viscous plasma incorporating the effect of thermal conductivity for star formation in interstellar medium (ISM)....
| Main Author: | |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
AIP Publishing LLC
2016-08-01
|
| Series: | AIP Advances |
| Online Access: | http://dx.doi.org/10.1063/1.4961991 |