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      Energetic Particles of Cosmic Accelerators I: Galactic Accelerators

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          Abstract

          The high-energy universe has revealed that energetic particles are ubiquitous in the cosmos and play a vital role in the cultivation of cosmic environments on all scales. Energetic particles in our own galaxy, galactic cosmic rays (GCRs), engage in a complex interplay with the interstellar medium and magnetic fields in the galaxy, giving rise to many of its key characteristics. This White Paper is the first of a two-part series highlighting the most well-known high-energy cosmic accelerators and contributions that MeV gamma-ray astronomy will bring to understanding their energetic particle phenomena. The focus of this white paper is galactic cosmic rays, supernova remnants, protostellar jets and superbubbles, and colliding wind binaries.

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          Detection of the Characteristic Pion-Decay Signature in Supernova Remnants

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            THREE-DIMENSIONAL INTEGRAL FIELD OBSERVATIONS OF 10 GALACTIC WINDS. I. EXTENDED PHASE (≳10 Myr) OF MASS/ENERGY INJECTION BEFORE THE WIND BLOWS

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              The OLS-lens survey the discovery of five new galaxy-galaxy strong lenses from the SDSS

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                Author and article information

                Journal
                11 March 2019
                Article
                1903.04634
                329e71b2-c0ea-45fb-8368-7506157fd93d

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

                History
                Custom metadata
                9 pages (including references), 2 figures; Submitted to the Astro2020 call for science white papers
                astro-ph.HE astro-ph.GA astro-ph.SR

                Galaxy astrophysics,High energy astrophysical phenomena,Solar & Stellar astrophysics

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