Paper Title |
Page |
Authors |
|
| |
Evolution of the X-Ray Properties of Clusters of Galaxies |
5 |
Henry, J. P. |
High Resolution X-Ray Spectroscopic Constraints on Cooling Flow Models of Clusters of Galaxies and Gaseous Haloes Around Elliptical Galaxies |
23 |
Kahn, S. M.; Peterson, J. R.; Paerels, F. B. S.; Xu, H.; Kaastra, J. S.; Ferrigno, C.; Tamura, T.; Bleeker, J.; Jernigan, J. G. |
A High Resolution Picture of the Intracluster Gas |
37 |
Markevitch, M.; Vikhlinin, A.; Forman, W. R. |
Chandra Observations of Relaxed Galaxy Clusters |
53 |
Allen, S. W. |
A Cold Front in A3667: Hydrodynamics and Magnetic Field in the Intracluster Medium |
63 |
Vikhlinin, A.; Markevitch, M. |
X-Ray observations of Galaxy Clusters and Cosmological Implications |
73 |
Böhringer, H.; Matsushita, K.; Finoguenov, A. |
Structural and Scaling Properties of the X-Ray Cluster Population and their Cosmological Implications |
85 |
Arnaud, M. |
Ωm and σ8 from the Abundance and Clustering of REFLEX Clusters of Galaxies |
97 |
Schuecker, Peter; Böhringer, H. |
High Energy Results from BeppoSAX |
109 |
Fusco-Femiano, R.; dal Fiume, D.; Orlandini, M.; de Grandi, S.; Molendi, S.; Feretti, L.; Grandi, P.; Giovannini, G. |
EUV Emission in Clusters of Galaxies |
125 |
Bowyer, S. |
Radio Observations of Clusters of Galaxies |
143 |
Feretti, L. |
The Fate of Intracluster Radio Plasma |
159 |
Enßlin, T. A. |
The Strength and Origins of Magnetic Fields In and Beyond Clusters |
169 |
Kronberg, P. P. |
Magnetic Fields in Clusters of Galaxies; Observational Results |
185 |
Clarke, T. E. |
Modeling Magnetic Fields in Galaxy Clusters |
193 |
Dolag, K. |
Gamma Rays from Clusters of Galaxies |
203 |
Blasi, P. |
Galaxy Evolution in Clusters |
221 |
Ellingson, E. |
Large Scale Environmental Effects in Clusters of Galaxies |
235 |
Kodama, T.; Smail, I.; Nakata, F.; Okamura, S.; Bower, R. G. |
Environment Shaping Galaxies: Star Formation Histories of Cluster Galaxies |
245 |
Poggianti, B. M. |
Strong and Weak Lensing by Galaxy Clusters |
255 |
Bartelmann, M. |
Wide-Field Weak Lensing Cluster Mass Reconstructions |
271 |
Clowe, D. |
The Most Massive Clusters in the Universe |
281 |
Czoske, Oliver; Kneib, Jean-Paul; Bardeau, Sébastien |
Cosmic Rays in Clusters of Galaxies |
293 |
Biermann, P. L.; Enßlin, T. A.; Kang, H.; Lee, H.; Ryu, D. |
Structure Shocks as a Source of Cosmic Rays in Clusters |
313 |
Jones, T. W.; Miniati, F.; Ryu, D.; Kang, H.; Hallman, E. J. |
Dynamical Role of Cosmic Rays in Clusters of Galaxies |
327 |
Ryu, D.; Kang, H.; Biermann, P. L. |
Nonthermal Radiation and Acceleration of Electrons in Clusters of Galaxies |
337 |
Petrosian, V. |
Modelling the Non-Thermal Emission from Galaxy Clusters |
349 |
Brunetti, G. |
Analytic Approaches to Understanding the Distribution of Intracluster Gas |
365 |
Wu, Xiang-Ping |
Density Profiles and Clustering of Dark Halos and Clusters of Galaxies |
379 |
Suto, Y. |
Quasi-stationary Cooling Flows with Small Mass Deposition |
395 |
Churazov, E. |
Pressure Balance between Thermal and Non-Thermal Plasmas in the 3C129 Cluster |
405 |
Harris, D. E.; Krawczynski, H. |
Cosmological Simulations of X-Ray Clusters: The Quest for Higher Resolution and Essential Physics |
419 |
Norman, M. |
The Peculiar Cooling Flow Cluster RX J0820.9+0752 |
437 |
Bayer-Kim, C. M.; Crawford, C. S.; Allen, S. W.; Fabian, A. C.; Edge, A. C. |
New Insights on Merging Clusters of Galaxies from XMM-Newton Observations |
443 |
Belsole, E.; Arnaud, M.; Chièze, J.-P.; Pratt, G. W.; Sauvageot, J.-L.; Ferrari, C.; Benoist, C.; Bourdin, H.; Maurogordato, S. |
Optically-selected clusters at 0.8 ≲ z ≲ 1.3 in the EIS Cluster Survey |
451 |
Benoist, C.; Neumann, D.; Arnaud, M.; da Costa, L.; Arnouts, S.; Jørgensen, H. E.; Olsen, L. F.; Bardelli, S.; Zucca, E.; Scodeggio, M.; Biviano, A.; Ramella, M. |
An Analysis of Claims of Detection of EUV Excesses with BeppoSAX; A Reanalysis |
457 |
Berghöfer, T.; Bowyer, Stuart |
Environmental Effects on the Galaxy Luminosity Function in the Cluster of Galaxies Abell 496 |
465 |
Durret, F.; Adami, C.; Lobo, C. |
The Line of Sight Mass Distribution Towards Gravitationally Lensed Quasar |
471 |
Faure, Cécile |
Chandra Observations of the Disruption of the Cool Core in Abell 133 |
477 |
Fujita, Y.; Sarazin, C. L.; Kempner, J. C.; Rudnick, L.; Slee, O. B.; Roy, A. L.; Andernach, H.; Ehle, M. |
Spectral Properties of Radio Halos |
483 |
Giovannini, G.; Feretti, L.; Bacchi, M.; Govoni, F. |
Modeling Radio Mini-Halos in Cooling Flow Clusters |
489 |
Gitti, M.; Brunetti, G.; Setti, G.; Feretti, L. |
First Results From an X-Ray, Weak Lensing and Sunyaev-Zeldovich Effect Survey of Nearby Clusters: Abell 3266 |
495 |
Gómez, P. L.; Romer, K. A.; Peterson, J.; Cantalupo, C.; Holzapfel, B.; Kuo, C.-L.; Newcomb, M.; Ruhl, J.; Goldstein, J.; Torbet, E.; Runyan, M. |
Magnetic Fields in Clusters of Galaxies Obtained Through the Study of Faraday Rotation Measures |
501 |
Govoni, F.; Feretti, L.; Murgia, M.; Taylor, G.; Giovannini, G.; Dallacasa, D. |
Reliability of the Dark Matter Clustering in Cosmological N-body Simulation on Scales Below the Mean Separation Length of Particles |
507 |
Hamana, T.; Yoshida, N.; Suto, Y. |
X-Ray Analysis of the MS0302 Supercluster |
513 |
Horner, D. J.; Donahue, M. |
Particle Acceleration Processes in the Coma Cluster |
519 |
Kuo, P.-H.; Hwang, C.-Y.; Ip, W.-H. |
XMM-Newton and Chandra view of the Cluster Abell 85 and its X-Ray Filament |
525 |
Lima Neto, G. B.; Durret, F. |
XMM-Newton AO-1 Observations Three SHARC Galaxy Clusters |
531 |
Majerowicz, S.; Arnaud, M.; Neumann, D. M. |
Weak Lensing Study of Abell 2029 |
537 |
Ménard, B.; Erben, T.; Mellier, Y. |
Multi-band Deep Optical Imagings of the Hickson Compact Groups |
543 |
Nishiura, S.; Shioya, Y.; Taniguchi, Y. |
Magneto-Turbulent Cosmic Ray Acceleration in Galaxy Clusters |
549 |
Ohno, H.; Takizawa, M.; Shibata, S. |
XMM-Newton Observation of A1413 |
555 |
Pratt, G. W.; Arnaud, M. |
On the Determination of the Mean Cosmic Matter Density and the Amplitude of Density Fluctuations |
563 |
Reiprich, T. H. |
Self-Gravitating Cooling Flows |
569 |
Wang, C.-Y.; Foster, P. N.; Ip, W.-H. |