Highly Energetic Physical Processes and Mechanisms for Emission from Astrophysical Plasmas: IAU Symposium 195

By S. Tsuruta. 2000

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Intergalactic Magnetic Fields from Quasar Outflows (2001, background): “…also account for the coherent field structure which is observed in galactic disks (Daly & Loeb 1990; Howard & Kulsrud 1997; note that supernova-driven outflows cannot reach the same level of coherence), and explain the large magnetic flux which is observed in X-ray clusters (Colgate & Li 2000).”
Light Curve and Spectral Models for the Hypernova SN 1998bw Associated with GRB 980425 (2000, background): “Subject headings: gamma-ray burst — supernovae — supernovae: individual (SN1998bw) — nucleosynthesis”
Particle acceleration and kinematics in solar flares – A Synthesis of Recent Observations and Theoretical Concepts (Invited Review) (2002, background): “The highest temperature of spectrally resolved thermal emission was measured at T ≈ 34 MK, using germanium-cooled detectors on a balloon-borne experiment (Lin et al. 1981). The thermal component dominates the hard X-ray spectrum only at low energies, up to 25 keV. So, the hard X-ray spectrum between”