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Guiding the Way to Gamma-Ray Sources: X-ray Studies of Supernova Remnants

Patrick Slane
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Abstract

Supernova remnants have long been suggested as a class of potential counterparts to unidentified gamma-ray sources. The mechanisms by which such gamma-rays can arise may include emission from a pulsar associated with a remnant, or a variety of processes associated with energetic particles accelerated by the SNR shock. Imaging and spectral observations in the X-ray band can be used to identify properties of the remnants that lead to gamma-ray emission, including the presence of pulsar-driven nebulae, nonthermal X-ray emission from the SNR shells, and the interaction of SNRs with dense surrounding material.

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Patrick Slane. 2001-04-21. Guiding the Way to Gamma-Ray Sources: X-ray Studies of Supernova Remnants. https://arxiv.org/abs/astro-ph/0104348

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