XMM-Newton observation of M87 I. Single-phase temperature structure of intracluster medium
Kyoko Matsushita, E. Belsole, A. Finoguenov, Hans Böhringer
Abstract
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Kyoko Matsushita, E. Belsole, A. Finoguenov, Hans Böhringer
Abstract
Open-access reader
We report the results of a detailed analysis of the temperature structure of the X-ray emitting plasma halo of M~87, the cD galaxy of the Virgo Cluster. Using the MEKAL model, the data provide strong indications that the intracluster medium has a single phase structure locally, except the regions associated to the radio structures. The deprojected spectrum at each radius is well fitted by a single temperature MEKAL model, except for the very central region ($
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We report the results of a detailed analysis of the temperature structure of the X-ray emitting plasma halo of M~87, the cD galaxy of the Virgo Cluster. Using the MEKAL model, the data provide strong indications that the intracluster medium has a single phase structure locally, except the regions associated to the radio structures. The deprojected spectrum at each radius is well fitted by a single temperature MEKAL model, except for the very central region ($
Key concepts: Intracluster medium, Physics, Cooling flow, Astrophysics, Virgo Cluster, Galaxy cluster, Gravitational potential, Type-cD galaxy