Abstract
We examine some aspects of the alignment of silicate dust grains with respect to the interstellar magnetic field. First, we consider possible observational constraints on the magnetic properties of the grains. Second, we investigate the role of collisions with gas atoms and the production of H2 molecules on the grain surface in the alignment process when the grain is drifting in the gaseous medium.
Author and committee
dc:creator, dc:contributor.*- Author
-
- Das, Indrajit
Subjects
dc:subject × 7Identifiers
dc:identifier.*- Identifier
- hdl:1920/8784
- OAI identifier oai:identifier
- oai:MARS:1920/8784