no code implementations • 10 Dec 2020 • P. Predehl, R. A. Sunyaev, W. Becker, H. Brunner, R. Burenin, A. Bykov, A. Cherepashchuk, N. Chugai, E. Churazov, V. Doroshenko, N. Eismont, M. Freyberg, M. Gilfanov, F. Haberl, I. Khabibullin, R. Krivonos, C. Maitra, P. Medvedev, A. Merloni, K. Nandra, V. Nazarov, M. Pavlinsky, G. Ponti, J. S. Sanders, M. Sasaki, S. Sazonov, A. W. Strong, J. Wilms
The halo of the Milky Way provides a laboratory to study the properties of the shocked hot gas that is predicted by models of galaxy formation.
Astrophysics of Galaxies High Energy Astrophysical Phenomena
1 code implementation • 10 May 2016 • J. S. Sanders, A. C. Fabian, H. R. Russell, S. A. Walker, K. M. Blundell
The effects of many physical processes in the intracluster medium of galaxy clusters imprint themselves in X-ray surface brightness images.
Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies High Energy Astrophysical Phenomena
