Results 81 to 90 of about 9,517 (211)
H.E.S.S. observations of the supernova remnant RCW 86 [PDF]
, 2007 S. Hoppe, M. Lemoine‐Goumard
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The Astrophysical JournalThe maximum energy of electrons in supernova remnant (SNR) shocks is typically limited by radiative losses, where the synchrotron cooling time equals the acceleration time.
Vincenzo Sapienza +7 more
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Interactions of particles accelerated in supernova remnants. Gamma-ray emission [PDF]
, 2013 O. Petruk, Vasyl Beshley
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Supernovae and the Arrow of Time. [PDF]
Entropy (Basel), 2022 Abarzhi SI +4 more
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MAGIC J0616+225 as delayed TeV emission of cosmic rays diffusing from the supernova remnant IC 443 [PDF]
, 2008 D. F. Torres +2 more
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Continuous solutions of cosmic-rays and waves in astrophysical environments. [PDF]
Sci Rep, 2023 Irshad K +5 more
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Cosmic-ray acceleration in a supernova remnant shock propagating in a stellar wind with a wind termination shock [PDF]
, 2023 Shoma F. Kamijima, Yutaka Ohira
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Nonthermal Signatures of Radiative Supernova Remnants
The Astrophysical JournalThe end of supernova remnant (SNR) evolution is characterized by a so-called “radiative” stage, in which efficient cooling of the hot bubble inside the forward shock slows expansion, leading to eventual shock breakup.
Rebecca Diesing +4 more
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A persistent influence of supernovae on biodiversity over the Phanerozoic. [PDF]
Ecol Evol, 2023 Svensmark H.
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Constraints of age, distance and progenitor of the supernova remnant RX\n J0852-4622/GRO J0852-4642 [PDF]
, 1999 B. Aschenbach +2 more
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