Sputtering of Amorphous Carbon Grains in a Cool Stellar Outflow

Details Sputtering of Amorphous Carbon Grains in a Cool Stellar Outflow Sputtering of Amorphous Carbon Grains in a Cool Stellar Outflow

Oct 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aps..4cf..ee03c&link_type=abstract

American Physical Society, Four Corners Section Fall Meeting, October 1-2, 1999 The University of Arizona Tucson, AZ, abstract #

Physics

Scientific paper

The outflows of cool stars are driven by radiation pressure on the dust component which transfers momentum to the gas component through collisions. The gas and dust are treated as a two component fluid and the outflow is assumed to be stationary. We follow the evolution of a size distribution of amorphous carbon grains that is being modified by nonthermal sputtering.

Affiliated with

Also associated with

No associations

Rating

Sputtering of Amorphous Carbon Grains in a Cool Stellar Outflow 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 Sputtering of Amorphous Carbon Grains in a Cool Stellar Outflow, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Sputtering of Amorphous Carbon Grains in a Cool Stellar Outflow will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1084152