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

Feb 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992nascp3137..388h&link_type=abstract

In NASA. Goddard Space Flight Center, The Compton Observatory Science Workshop p 388-396 (SEE N92-21874 12-90)

Statistics

Computation

2

Estimates, Gamma Ray Spectrometers, Gamma Rays, Monte Carlo Method, Signatures, Supernovae, Computational Astrophysics, Constraints, Emission Spectra, Gamma Ray Astronomy, Heao 3

Scientific paper

Monte Carlo simulations of the expected gamma-ray signatures of galactic supernovae of all types are performed in order to estimate the significance of the lack of a gamma-ray signal due to supernovae occurring during the last millenium. Using recent estimates of nuclear yields, we determine 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.

Affiliated with

Also associated with

No associations

Rating

Gamma ray constraints on the galactic supernova rate does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Gamma ray constraints on the galactic supernova rate, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gamma ray constraints on the galactic supernova rate will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1050651