Acceleration of supernovae envelopes by pulsar produced radiation

Details Acceleration of supernovae envelopes by pulsar produced radiation Acceleration of supernovae envelopes by pulsar produced radiation

Dec 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mmsai..49..817b&link_type=abstract

(Consiglio Nazionale delle Ricerche, Convegno sulle Metodologie di Trattamento dell'Informazione, Trieste, Nov. 24, 25, 1977 and

Physics

Crab Nebula, Pulsars, Stellar Envelopes, Stellar Motions, Stellar Radiation, Supernovae, Acceleration (Physics), Synchrotron Radiation

Scientific paper

A theoretical analysis of the general pulsar kinematics and supernova envelope dynamics is presented. It is found that over a period of several months after the collapse of a supernova the entire radiation energy output of the resulting pulsar will be absorbed by the envelope, first arresting the inward motion of the latter, then forcing its expulsion.

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