Gamma ray constraints on the Galactic supernova rate

Details Gamma ray constraints on the Galactic supernova rate Gamma ray constraints on the Galactic supernova rate

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991sdgg.nasa.....h&link_type=abstract

In its Gamma-Ray Spectroscopy: The Diffuse Galactic Glow 9 p (SEE N92-16968 07-93)

Other

Estimates, Galactic Radiation, Gamma Rays, Monte Carlo Method, Signatures, Supernovae, Constraints, Emission, Gamma Ray Spectrometers, Heao 3, Rates (Per Time), Simulation, Surveys

Scientific paper

We perform Monte Carlo simulations of the expected gamma ray signatures of Galactic supernovae of all types to estimate the significance of the lack of a gamma ray signal due to supernovae occurring during the last millenium. Using recent estimates of the nuclear yields, we determine mean Galactic supernova rates consistent with the historic supernova record and the gamma ray limits. Another objective of these calculations of Galactic supernova histories is their application to surveys of diffuse Galactic gamma ray line emission.

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