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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.
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Nency R. Patel, Mathilde Jauzac,Anna Niemiec,David Lagattuta,Guillaume Mahler,Benjamin Beauchesne,Alastair Edge,Harald Ebeling,Marceau Limousin
arxiv(2024)
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Arthur Whyley,Scott W. Randall,Tracy E. Clarke, Reinout J. van Weeren,Kamlesh Rajpurohit,William R. Forman,Alastair C. Edge,Elizabeth L. Blanton,Lorenzo Lovisari,Huib T. Intema
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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V. A. Fawcett,D. M. Alexander,A. Brodzeller,A. C. Edge,D. J. Rosario,A. D. Myers,J. Aguilar, S. Ahlen, R. Alfarsy,D. Brooks, R. Canning, C. Circosta,
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYno. 4 (2023): 5575-5596
arXiv (Cornell University) (2023)
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Monthly Notices of the Royal Astronomical Society (2023)
arxiv(2023)
arxiv(2023)
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