Possible mass distributions in the nebulae of other solar systems

Details Possible mass distributions in the nebulae of other solar systems Possible mass distributions in the nebulae of other solar systems

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987em%26p...37..225b&link_type=abstract

Earth, Moon, and Planets (ISSN 0167-9295), vol. 37, March 1987, p. 225-239.

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2

Astronomical Models, Extrasolar Planets, Interplanetary Medium, Mass Distribution, Nebulae, Solar System, Shear Flow, Stellar Rotation, Supernovae

Scientific paper

Mass distributions of other solar nebulae are calculated using the supernova shell fragmentation model of solar system formation. The variable a, expressing the ratio of shear flow to the rotation of the supernova star, is found to be crucial to the shape of the mass distributions, though the limits on a are not well established and the range of a may have been overestimated. Disc mass distributions are calculated with the SOLSYS program (Brown and Gritzo, 1987) for various values of (b/r)tan theta, in which 2b is the height and r is the radius of the cylindrical fragment.

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