Search Results - "Das, Samata"
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Leptonic Nonthermal Emission from Supernova Remnants Evolving in the Circumstellar Magnetic Field
Published in The Astrophysical journal (01-02-2022)“…Abstract The very-high-energy (VHE; E > 100 GeV) gamma-ray emission observed from a number of supernova remnants (SNRs) indicates particle acceleration to high…”
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Production of secondary particles in heavy nuclei interactions in supernova remnants
Published in Astroparticle physics (01-12-2020)“…Depending on their type, supernova remnants may have ejecta material with high abundance of heavy elements such as carbon or oxygen. In addition, core-collapse…”
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Particle acceleration, escape and non-thermal emission from core-collapse supernovae inside non-identical wind-blown bubbles
Published 28-08-2024“…A&A, 689 (2024) A9 In the core-collapse scenario, the supernova remnants evolve inside the complex wind-blown bubbles, structured by massive progenitors during…”
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Leptonic non-thermal emission from supernova remnants evolving in the circumstellar magnetic field
Published 23-11-2021“…The very-high-energy (VHE; E > 100 GeV) gamma-ray emission observed from a number of Supernova remnants (SNRs) indicates particle acceleration to high energies…”
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Journal Article -
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Spectral softening in core-collapse supernova remnant expanding inside wind-blown bubble
Published 07-03-2022“…A&A 661, A128 (2022) Context. Galactic cosmic rays are widely assumed to arise from diffusive shock acceleration, specifically at shocks in supernova remnants…”
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6
Production of secondary particles in heavy nuclei interactions in supernova remnants
Published 08-07-2020“…Depending on their type, supernova remnants may have ejecta material with high abundance of heavy elements such as carbon or oxygen. In addition, core-collapse…”
Get full text
Journal Article