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Dark matter (DM) dominates the properties of large cosmological structures such as galaxy clusters, and the mass profiles of the DM have been inferred for these equilibrated structures for years by using cluster X-ray surface brightnesses and tempera
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::052ece68fbf8d162178db08550f4d875
https://ora.ox.ac.uk/objects/uuid:ef95feaf-ef45-4ba4-aff3-67f60398ed62
https://ora.ox.ac.uk/objects/uuid:ef95feaf-ef45-4ba4-aff3-67f60398ed62
