Ancient cosmic ray halos from the central galaxy boost Perseus's cool core via inverse-Compton scattering, simultaneously explaining radio minihalo, giant halo, X-ray properties, and gamma-ray data without re-acceleration.
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VERITAS and multiwavelength observations of the 2017 NGC 1275 gamma-ray flare show harder-when-brighter spectral evolution and support a two-component jet model with 10-degree viewing angle and gamma-ray emission near the C3 radio component.
citing papers explorer
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An Inverse-Compton-Boosted Cool Core Unifies Perseus's Radio and X-ray Halos
Ancient cosmic ray halos from the central galaxy boost Perseus's cool core via inverse-Compton scattering, simultaneously explaining radio minihalo, giant halo, X-ray properties, and gamma-ray data without re-acceleration.
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The exceptional 2017 gamma-ray flare of the radio galaxy NGC 1275: VERITAS and Multiwavelength Observations
VERITAS and multiwavelength observations of the 2017 NGC 1275 gamma-ray flare show harder-when-brighter spectral evolution and support a two-component jet model with 10-degree viewing angle and gamma-ray emission near the C3 radio component.