The combined effects of supernova explosions and stellar winds produce a hot bubble in the central
regions of starburst galaxies. As the bubble expands, it can outbreak into the galactic halo driving a
superwind that transports hot gas and fields to the intergalactic space. We present estimates of cosmic
ray generation and gamma-ray emission in both this large-scale wind and the bow shocks created around the embedded clouds.
Volume 354 -
High Energy Phenomena in Relativistic Outflows VII (HEPRO VII) -
Relativistic outflows from extragalactic sources
Gamma-Rays From Large-Scale Outflows In Starburst Galaxies
Full text:
pdf
Published on:
February 25, 2020
Abstract
DOI: https://doi.org/10.22323/1.354.0029
How to cite
Metadata are provided both in "article" format (very similar to INSPIRE) as this helps creating very compact bibliographies which can be beneficial to authors and readers, and in "proceeding" format which is more detailed and complete.
Open Access
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.