A method for predicting the soft X-ray flux from supernovae

Details A method for predicting the soft X-ray flux from supernovae A method for predicting the soft X-ray flux from supernovae

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...230..742l&link_type=abstract

Astrophysical Journal, Part 1, vol. 230, June 15, 1979, p. 742-754.

Astronomy and Astrophysics

Astrophysics

20

Flares, Interstellar Extinction, Radiant Flux Density, Stellar Envelopes, Supernovae, X Ray Sources, Electromagnetic Absorption, Gas Explosions, Prediction Analysis Techniques

Scientific paper

This paper gives a set of predictions of the properties of the soft X-ray flare from supernovae based on the energy of the explosion and the characteristics of the envelope of the star. The effects of the absorption of the interstellar medium are included to determine the photon flux, time duration, and average photon energy of the received radiation. The method is expressed in a number of simple approximate relationships which can be used to find the predicted quantities for any set of input values.

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