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- W2403367155 abstract "The origin of the radio halo in the Coma cluster is discussed here. Particular attention is paid to the galactic wake theory: the wakes are assumed to be turbulent and able to reaccelerate particles via either first-order Fermi or the Eilek-Henriksen mechanism. The expected energetics driven from the theory is in good agreement with the observed data. The need for particle acceleration processes, especially first-order Fermi type, is emphasized. The rarity of Comatype radio halos is considered to be due to either an insufficient particle supply or to the fact that particles in their ICM are not old (< 1010 y) enough to produce a halo as extended as that in the Coma cluster of galaxies." @default.
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- W2403367155 date "1990-08-01" @default.
- W2403367155 modified "2023-09-27" @default.
- W2403367155 title "On the origin of the radio halo in the coma cluster of galaxies" @default.
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- W2403367155 doi "https://doi.org/10.1007/bf02741552" @default.
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