Gamma-ray line emission from supernova remnants

Details Gamma-ray line emission from supernova remnants Gamma-ray line emission from supernova remnants

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..565..173m&link_type=abstract

YOUNG SUPERNOVA REMNANTS: Eleventh Astrophysics Conference. AIP Conference Proceedings, Volume 565, pp. 173-176 (2001).

Astronomy and Astrophysics

Astrophysics

Gamma-Ray, Supernova Remnants

Scientific paper

Gamma-ray line emission from the decays of radio-isotopes produced in supernovae should be detectable by three future gamma-ray telescopes. The 511 keV, 1157 keV, 1173 keV and 1809 keV lines produced in young supernova remnants are a powerful probe of the mass yields and ejecta kinematics of these objects. Nineteen supernova remnants have been studied to determine which gamma-ray lines will be detected by these three instruments. The results of this study and the scientific potential of these observations are discussed. .

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