Dynamics of self-gravitating shells driven by radiation pressure from the field stars

Details Dynamics of self-gravitating shells driven by radiation pressure from the field stars Dynamics of self-gravitating shells driven by radiation pressure from the field stars

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988kfnt....4...85p&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 4, Mar.-Apr. 1988, p. 85-87. In Russian.

Physics

2

Radiation Pressure, Stellar Envelopes, Stellar Gravitation, Stellar Radiation, Acceleration (Physics), Star Distribution, Stellar Evolution, Stellar Motions

Scientific paper

It is shown that self-gravitating shells can be accelerated only when the energy density of the stellar radiation exceeds the critical value of 3.6 x 10 to the -13th J/cu m. It is thus concluded that the acceleration mechanism for self-gravitating shells connected with radiation pressure from the field stars is not effective for systems with Galaxy parameters.

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