The Radial Mass Distribution Due to Heating Events

Details The Radial Mass Distribution Due to Heating Events The Radial Mass Distribution Due to Heating Events

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1724k&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1724

Physics

Scientific paper

Heating events in the solar nebula were localized in 3D, on the order of
the scale height for the gas. This idea, combined with a changing of the
'surface' of the nebula in response to the event, predicts the observed
projected surface density.

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