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Monthly notices of the Royal Astronomical Society, ISSN 1365-2966, 08/2014, Volume 442, Issue 3, pp. 2048 - 2057
Emission from the active nucleus in the core of the brightest cluster galaxy of the Perseus cluster, NGC 1275, has varied dramatically over the past four... 
radiation mechanisms: non-thermal | galaxies: clusters: individual: Perseus | gamma rays: galaxies - radio continuum: galaxies | galaxies: individual: NGC 1275 | galaxies: active | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Physics - High Energy Astrophysical Phenomena
Journal Article
Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, 2017, Volume 467, Issue 2, pp. 1478 - 1495
... and dissipation of resonantly generated Alfven waves and by thermal conduction at large radii. Here, we demonstrate that the predicted non-thermal emission resulting... 
Galaxies: clusters: general | Radiation mechanisms: non-thermal | Conduction | Galaxies: active | Cosmic rays | Physical Sciences | Astronomy & Astrophysics | Science & Technology
Journal Article
Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, 2017, Volume 471, Issue 1, pp. L150 - L154
HESS J0632+057 is an eccentric gamma-ray Be binary that produces non-thermal radio, Xrays, GeV and very high-energy gamma-rays... 
Radiation mechanisms: non-thermal | Hydrodynamics | Stars: winds, outflows | Gamma-rays: stars -X-rays: binaries | Physical Sciences | Astronomy & Astrophysics | Science & Technology
Journal Article
Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, 02/2019, Volume 482, Issue 4, pp. 4630 - 4641
.... The spectral index of the emission in the shell is -0.8, indicating non-thermal emission. H alpha emission that mimics the morphology of the radio shell on a smaller scale is also detected here... 
Infrared: ISM | ISM: Individual objects: SNR 351.7−1.2 | Radiation mechanisms: Non-thermal | H II regions | ISM: Supernova remnants | Physical Sciences | Astronomy & Astrophysics | Science & Technology
Journal Article
Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, 07/2012, Volume 423, Issue 4, pp. 3512 - 3539
Journal Article