Cosmological MHD simulation of a cooling flow cluster

Astronomy and Astrophysics

Volumn 482, Issue 2, 2008, Pages

  Dubois, Y ^a   Teyssier, R ^a  

^a DIF   (France)

Author keywords

Galaxies: clusters: general; Galaxies: cooling flows; Galaxies: magnetic fields; Methods: numerical

Indexed keywords

AMPLIFICATION; COOLING; COSMIC RAYS; MAGNETIC FIELDS; SYNCHROTRON RADIATION;

COOLING FLOW CLUSTERS; GALAXY CLUSTERS; MAGNETIC RECONNECTION; SPATIAL STRUCTURE;

GALAXIES;

EID: 42349084835     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200809513     Document Type: Article

References (22)

1. Asai, N., Fukuda, N., & Matsumoto, R. 2007, ApJ, 663, 816
2. Brüggen, M., Ruszkowski, M., Simionescu, A., Hoeft, M., & Dalla Vecchia, C. 2005, ApJ, 631, L21
3. Brunetti, G., & Lazarian, A. 2007, MNRAS, 378, 245
4. Clarke, T. E., Kronberg, P. P., & Böhringer, H. 2001, ApJ, 547, L111
5. Dolag, K. 2000, in Constructing the Universe with Clusters of Galaxies
6. Dolag, K., Bartelmann, M., & Lesch, H. 1999, A&A, 348, 351
7. Dolag, K., Grasso, D., Springel, V., & Tkachev, I. 2005, J. Cosmol. Astro-Particle Phys., 1, 9
8. Fromang, S., Hennebelle, P., & Teyssier, R. 2006, A&A, 457, 371
9. Globus, N., Allard, D., & Parizot, E. 2007, ArXiv e-prints, 709
10. Govoni, D., & Feretti, L. 2004, Int. J. Mod. Phys. D, 13, 1549
11. Haardt, F., & Madau, P. 1996, ApJ, 461, 20
12. Jones, T. W. 2007, ArXiv e-prints, 708
13. King, E. J., & Coles, P. 2006, MNRAS, 365, 1288
14. Kotera, K., & Lemoine, M. 2008, Phys. Rev. D, 77, 023005
15. Lemoine, M. 2005, Phys. Rev. D, 71, 083007
16. Miniati, F., Jones, T. W., Kang, H., & Ryu, D. 2001, ApJ, 562, 233
17. Miyoshi, T., & Kusano, K. 2005, J. Computational Phys., 208, 315
18. Roettiger, K., Stone, J. M., & Burns, J. O. 1999, ApJ, 518, 594
19. Sigl, G., Miniati, F., & Enßlin, T. A. 2004, Phys. Rev. D, 70, 043007
20. Taylor, G. B., Fabian, A. C., & Allen, S. W. 2002, MNRAS, 334, 769
21. Teyssier, R. 2002, A&A, 385, 337
22. Teyssier, R., Fromang, S., & Dormy, E. 2006, J. Computational Phys., 218, 44