Search Results - "Das, Samata"

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  1. 1

    Leptonic Nonthermal Emission from Supernova Remnants Evolving in the Circumstellar Magnetic Field by Sushch, Iurii, Brose, Robert, Pohl, Martin, Plotko, Pavlo, Das, Samata

    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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    Journal Article
  2. 2

    Production of secondary particles in heavy nuclei interactions in supernova remnants by Bhatt, Maulik, Sushch, Iurii, Pohl, Martin, Fedynitch, Anatoli, Das, Samata, Brose, Robert, Plotko, Pavlo, Meyer, Dominique M.-A.

    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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    Journal Article
  3. 3

    Particle acceleration, escape and non-thermal emission from core-collapse supernovae inside non-identical wind-blown bubbles by Das, Samata, Brose, Robert, Pohl, Martin, Meyer, Dominique M. -A, Sushch, Iurii

    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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    Journal Article
  4. 4

    Leptonic non-thermal emission from supernova remnants evolving in the circumstellar magnetic field by Sushch, Iurii, Brose, Robert, Pohl, Martin, Plotko, Pavlo, Das, Samata

    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
  5. 5

    Spectral softening in core-collapse supernova remnant expanding inside wind-blown bubble by Das, Samata, Brose, Robert, Meyer, Dominique M. -A, Pohl, Martin, Sushch, Iurii, Plotko, Pavlo

    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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    Journal Article
  6. 6

    Production of secondary particles in heavy nuclei interactions in supernova remnants by Bhatt, Maulik, Sushch, Iurii, Pohl, Martin, Fedynitch, Anatoli, Das, Samata, Brose, Robert, Plotko, Pavlo, Meyer, Dominique M. -A

    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