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- W2021357314 abstract "Superbubbles (SBs) are among the greatest injectors of energy into the Galaxy, and have been proposed to be the acceleration site of Galactic cosmic rays. They are thought to be powered by the fast stellar winds and powerful supernova explosions of massive stars in dense stellar clusters and associations. Observations of the SB DEM L192 in the neighboring Large Magellanic Cloud (LMC) show that it contains only about one-third the energy injected by its constituent stars via fast stellar winds and supernovae. It is not yet understood where the excess energy is going—thus, the so-called energy-crisis. We show here that it is very likely that a significant fraction of the unaccounted for energy is being taken up in accelerating cosmic rays, thus bolstering the argument for the SB origin of cosmic rays." @default.
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- W2021357314 date "2008-03-14" @default.
- W2021357314 modified "2023-09-26" @default.
- W2021357314 title "A Cosmic-Ray Resolution to the Superbubble Energy Crisis" @default.
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- W2021357314 doi "https://doi.org/10.1086/587875" @default.
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