Kinematic analysis of a sample of X-ray luminous distant galaxy clusters - the 
LX − σv relation in the z > 0.6 universe

Nastasi, A.; Böhringer, H.; Fassbender, R.; de Hoon, A.; Lamer, G.; Mohr, J. J.; Padilla, N.; Pratt, G. W.; Quintana, H.; Rosati, P.; Santos, J. S.; Schwope, A. D.; Šuhada, R.; Verdugo, M.

doi:10.1051/0004-6361/201322321

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Kinematic analysis of a sample of X-ray luminous distant galaxy clusters - the LX − σv relation in the z > 0.6 universe

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Nastasi, A.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Böhringer, H.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Fassbender, R.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Nastasi, A., Böhringer, H., Fassbender, R., de Hoon, A., Lamer, G., Mohr, J. J., Padilla, N., Pratt, G. W., Quintana, H., Rosati, P., Santos, J. S., Schwope, A. D., Šuhada, R., & Verdugo, M. (2014). Kinematic analysis of a sample of X-ray luminous distant galaxy clusters - the LX − σv relation in the z > 0.6 universe. Astronomy & Astrophysics, 564:, pp. 1-23. doi:10.1051/0004-6361/201322321.

引用: https://hdl.handle.net/11858/00-001M-0000-0019-CE8E-7

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