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astro-ph2004
Radiative cooling, heating and thermal conduction in M87
Simona Ghizzardi, Silvano Molendi, Fabio Pizzolato +1
The crisis of the standard cooling flow model brought about by Chandra and XMM-Newton observations of galaxy clusters, has led to the development of several models which explore di…
astro-ph2003
SMAUG: a new technique for the deprojection of galaxy clusters
F. Pizzolato, S. Molendi, S. Ghizzardi +1
This paper presents a new technique for reconstructing the spatial distributions of hydrogen, temperature and metal abundance of a galaxy cluster. These quantities are worked out f…