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Bio
My research concentrates on clusters of galaxies from an X-ray prespective. Selecting clusters on the basis of their X-ray luminosity ensures that the objects are massive and well-relaxed. In many cases these clusters are relatively dense in their cores and the resulting strong X-ray emission causes all the thermal energy of the gas to be radiated away. This phenomenon is termed a "Cooling Flow". The clear and unescapable conclusion from the X-ray observations is that there is a substantial mass of gas that has cooled but relatively little of this 'sink' had been found before 2000.
Research Interests
Papers共 526 篇Author StatisticsCo-AuthorSimilar Experts
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Tom Rose,B. R. McNamara,F. Combes,A. C. Edge, M. McDonald,Ewan O'Sullivan,H. Russell, A. C. Fabian,G. Ferland,P. Salome,G. Tremblay
arxiv(2024)
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arxiv(2024)
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MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYno. 2 (2024): 3441-3455
arxiv(2024)
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Benjamin Vigneron,Julie Hlavacek-Larrondo,Carter Lee Rhea,Marie-Lou Gendron-Marsolais,Jeremy Lim, Jake Reinheimer,Yuan Li,Laurent Drissen,Greg L. Bryan,Megan Donahue,Alastair Edge,Andrew Fabian,
arxiv(2024)
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arXiv (Cornell University) (2023)
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYno. 4 (2023): 5575-5596
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