Statistics of gravitational potential perturbations: A novel approach to deriving the X-ray temperature function
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Publication:3618888
DOI10.1051/0004-6361:200809562zbMath1160.85317arXiv0802.1680OpenAlexW2086596971WikidataQ59320673 ScholiaQ59320673MaRDI QIDQ3618888
C. Angrick, Matthias Bartelmann
Publication date: 3 April 2009
Published in: Astronomy & Astrophysics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/0802.1680
cosmology: theorygalaxies: clusters: generalmethods: analyticalcosmology: cosmological parameterscosmology: dark matterX-rays: galaxies: clusters
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