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The e-ASTROGAM space mission: a major step forward for supernova physics

Published online by Cambridge University Press:  17 October 2017

Vincent Tatischeff ,
Roland Diehl Open the ORCID record for Roland Diehl [Opens in a new window]  and
Alessandro De Angelis
Vincent Tatischeff
Affiliation:
CSNSM, IN2P3-CNRS/Univ. Paris-Sud, Université Paris-Saclay, F-91405 Orsay Campus, France email: vincent.tatischeff@csnsm.in2p3.fr
Roland Diehl
Affiliation:
Max Planck Institut für extraterrestrische Physik, D-85748 Garching, Germany email: rod@mpe.mpg.de
Alessandro De Angelis
Affiliation:
INFN Padova, via Marzolo 8, 35141, Padova, Italy LIP/IST, Av. Elias Garcia 14, 1000 Lisboa, Portugal email: alessandro.deangelis@pd.infn.it
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Abstract

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e-ASTROGAM is a gamma-ray observatory operating in a broad energy range, 0.15 MeV – 3 GeV, recently proposed as the M5 Medium-size mission of the European Space Agency. It has the potential to revolutionize the astronomy of medium-energy gamma-rays by increasing the number of known sources in this domain by more than an order of magnitude and providing gamma-ray polarization information for many of these sources. In these proceedings, we discuss the expected capacity of the mission to study the physics of supernovae, both thermonuclear and core-collapse, as well as the origin of cosmic rays in SN shocks.

Keywords

Gamma rays: observationstelescopesradiation mechanisms: nonthermalsupernovae: generalsupernova remnantscosmic rays
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S331: Supernova 1987A:30 years later - Cosmic Rays and Nuclei from Supernovae and their aftermaths , February 2017 , pp. 351 - 356
Copyright
Copyright © International Astronomical Union 2017 

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