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Titlebook: Merging Processes in Galaxy Clusters; L. Feretti,I. M. Gioia,G. Giovannini Book 2002 The Editor(s) (if applicable) and The Author(s), unde

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樓主: ergonomics
21#
發(fā)表于 2025-3-25 06:47:12 | 只看該作者
Gabriele Giovannini,Luigina Ferettiists from the Scientific Group Thermodata Europe (SGTE)..IncThermodynamic data for inorganic materials are fundamental for the optimisation of existing process parameters and for investigating suitable parameters for carrying out potential new processes. With the aid of such data, time and costs can
22#
發(fā)表于 2025-3-25 08:16:58 | 只看該作者
23#
發(fā)表于 2025-3-25 12:39:27 | 只看該作者
August E. Evrard,Isabella M. Gioiaists from the Scientific Group Thermodata Europe (SGTE)..IncThermodynamic data for inorganic materials are fundamental for the optimisation of existing process parameters and for investigating suitable parameters for carrying out potential new processes. With the aid of such data, time and costs can
24#
發(fā)表于 2025-3-25 18:59:52 | 只看該作者
ists from the Scientific Group Thermodata Europe (SGTE)..IncThermodynamic data for inorganic materials are fundamental for the optimisation of existing process parameters and for investigating suitable parameters for carrying out potential new processes. With the aid of such data, time and costs can
25#
發(fā)表于 2025-3-25 22:34:50 | 只看該作者
The Physics of Cluster Mergers, the Universe since the Big Bang. Some of the basic physical properties of mergers will be discussed, with an emphasis on simple analytic arguments rather than numerical simulations. Semi-analytic estimates of merger rates are reviewed, and a simple treatment of the kinematics of binary mergers is g
26#
發(fā)表于 2025-3-26 01:24:18 | 只看該作者
27#
發(fā)表于 2025-3-26 05:36:56 | 只看該作者
28#
發(fā)表于 2025-3-26 09:10:00 | 只看該作者
High Angular Resolution Cluster Observations with Chandra,arp, edge-like surface brightness structures in clusters. These sharp features, previously suggested to be shock fronts, probably arise from cluster mergers. We review Chandra observations of merging clusters with radio halos that provide new insights into the particle acceleration mechanisms for pr
29#
發(fā)表于 2025-3-26 15:36:25 | 只看該作者
30#
發(fā)表于 2025-3-26 16:52:13 | 只看該作者
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