New composite models of partially ionized protoplanetary disks
We study an accretion disk in which three different regions may coexist: MHD turbulent regions, dead zones and gravitationally unstable regions. Although the dead zones are stable, there is some transport due to the Reynolds stress associated with waves emitted from the turbulent layers. We model th...
| מחבר ראשי: | |
|---|---|
| פורמט: | Journal article |
| שפה: | English |
| יצא לאור: |
Institute of Physics Publishing
2008
|