Efficiency of Mixing of Supernova Ejecta into Nearby Protoplanetary Disks

Details Efficiency of Mixing of Supernova Ejecta into Nearby Protoplanetary Disks Efficiency of Mixing of Supernova Ejecta into Nearby Protoplanetary Disks

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.2348o&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.2348

Physics

2

Scientific paper

The one-time presence of 60Fe in our solar system implies it formed in
close proximity to a supernova. We investigate the effects of supernova
ejecta hitting a protoplanetary disk, and the efficiency with which
ejecta gas mixes into the disk.

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