Publikationen von K. Dolag
Alle Typen
Konferenzbeitrag (35)
361.
Konferenzbeitrag
Simulating the magnetic field in the local supercluster. In: X-Ray and Radio Connections, S. 1 - 6 (Hg. Sjouwerman, L.O.; Dyer, K.K.). X-Ray and Radio Connections, Santa Fe, New Mexico, 03. Februar 2004 - 06. Februar 2004. NRAO (2005)
362.
Konferenzbeitrag
Constraints on dark energy from strong gravitational lensing by galaxy clusters. In: Impact of Gravitational Lensing on Cosmology, S. 185 - 192 (Hg. Mellier, Y.; Meylan, G.). 225th Symposium of the International Astronomical Union, Lausanne, Switzerland, 19. Juli 2004 - 23. Juli 2004. Cambridge University Press, Cambridge, UK (2005)
363.
Konferenzbeitrag
The evolution of magnetic fields in galaxy clusters. In: Astrophysical supercomputing using particle simulations: Proceedings of the 208th symposium of the International Astronomical Union, S. 189 - 198 (Hg. Makino Hut Piet, J.). Astrophysical supercomputing using particle simulations, Tokyo, Japan, 10. Juli 2001 - 13. Juli 2001. Astronomical Society of the Pacific, San Francsisco, CA (US) (2003)
364.
Konferenzbeitrag
Modeling magnetic fields in galaxy clusters. In: Matter and energy in cluster of galaxies, S. 193 - 200 (Hg. Bowyer, S.; Hwang, C.-Y.). Matter and energy in cluster of galaxies, Chung-Li, Taiwan, 23. April 2002 - 27. April 2002. Astronomical Society of the Pacific, San Francisco, CA (US) (2003)
365.
Konferenzbeitrag
Simulating magnetic fields in galaxy clusters, a tool to learn more about this obscure ingredient of clusters. In: Clusters of galaxies and the high redshift universe observed in x-rays - Recent results of XMM-Newton and Chandra (Hg. Tranh Thanh Van, J.; Neumann, D. M.). XXIst Moriond astrophysics meeting / XXXVIth Rencontres de Moriond, Les Arcs, Sovoie, France, 10. März 2001 - 17. März 2001. CEA, Paris (2002)
Forschungspapier (1)
366.
Forschungspapier
The evolution of galaxy groups and clusters. The hot and energetic universe (2013), 9 S.
Bericht (1)
367.
Bericht
Die Vorhersage des Sunyaev-Zeldovich-Signals aus kosmologischen, hydrodynamischen Simulationen. (2017)