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Thermal radiation processes

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arxiv 0801.1011 v1 pith:M3YIJB7T submitted 2008-01-07 astro-ph

J.S. Kaastra , F.B.S. Paerels , F. Durret , S. Schindler , P. Richter This is my paper · ORCID
classification astro-ph
keywords absorptionemissionimportantprocessesspectrathermalx-raybalance
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We discuss the different physical processes that are important to understand the thermal X-ray emission and absorption spectra of the diffuse gas in clusters of galaxies and the warm-hot intergalactic medium. The ionisation balance, line and continuum emission and absorption properties are reviewed and several practical examples are given that illustrate the most important diagnostic features in the X-ray spectra.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 72 citations worldwide. Full citation record

  1. Spatially resolved optical and mid-infrared spectroscopy of SDSS1335+0728: implications for the origin of the Ansky event

    astro-ph.GA 2026-07 unverdicted novelty 7.0 of 10

    Spatially resolved spectroscopy shows SDSS1335+0728 has a three-zone ionisation structure, optically thin dust, and sustained low-level nuclear activity for at least 1500 years, implying the Ansky event is a faint tra...

  2. DIffuse X-ray Explorer (DIXE): Sky Survey Strategy and Collimator Response Demodulation

    astro-ph.IM 2026-06 unverdicted novelty 7.0 of 10

    DIXE proposes CSS-based survey strategies covering 72.5% of the sky with 26-68 ks exposures and shows via simulation that MCMC collimator demodulation yields 1° point-source localization and 3° extended-source resolution.

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