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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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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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Tom Rose,B. R. McNamara, F. Combes,A. C. Edge,H. Russell,P. Salome, P. Tamhane,A. C. Fabian,G. Tremblay
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYno. 2 (2024): 3441-3455
N. Biava,A. Bonafede, F. Gastaldello,A. Botteon,M. Brienza, T. W. Shimwell, G. Brunetti,L. Bruno,K. Rajpurohit,C. J. Riseley,R. J. van Weeren, M. Rossetti,
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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