Planet Formation Processes in a Marginally Gravitationally Unstable Disk Around a Solar-Mass Protostar

Details Planet Formation Processes in a Marginally Gravitationally Unstable Disk Around a Solar-Mass Protostar Planet Formation Processes in a Marginally Gravitationally Unstable Disk Around a Solar-Mass Protostar

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2205b&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2205

Physics

Scientific paper

Marginally gravitationally unstable disks provide a natural mechanism
for the rapid transport radially inward and outward of short-lived
radioactivities and refractory grains, but they might also form giant
planets by disk instability.

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