3D radiation MHD simulations of gas and dust in protoplanetary disks
Abstract
3D global radiation MHD simulations of gas and dust in protoplanetary disks allow us to understand the dynamical and thermal evolution of protoplanetary disks. At the same time, recent observations in the mm-dust emission by the Atacama Large Millimeter Array (ALMA) allow us to resolve structures at scales of the disk scale height.
- Publication:
-
Origins: From the Protosun to the First Steps of Life
- Pub Date:
- 2020
- DOI:
- 10.1017/S1743921319001923
- Bibcode:
- 2020IAUS..345..124F
- Keywords:
-
- MHD simulations;
- accretion disks;
- protoplanetary disks;
- mm observations