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pro vyhledávání: '"Neumann, D. A."'
Autor:
Neuman, V., Vavra, D., Drnkova, L., Pruhova, S., Plachy, L., Kolouskova, S., Obermannova, B., Amaratunga, S.A., Konecna, P., Vyzralkova, J., Venhacova, P., Pomahacova, R., Paterova, P., Stichova, L., Skvor, J., Kocourkova, K., Romanova, M., Vosahlo, J., Strnadel, J., Polockova, K., Neumann, D., Slavenko, M., Sumnik, Z.
Publikováno v:
In Diabetes Research and Clinical Practice February 2024 208
Akademický článek
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Akademický článek
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Autor:
Guzzo, L., Schuecker, P., Boehringer, H., Collins, C. A., Ortiz-Gil, A., De Grandi, S., Edge, A. C., Neumann, D. M., Schindler, S., Altucci, C., Shaver, P. A.
Publikováno v:
A&A, 2009, 499, 357
We present the final data from the spectroscopic survey of the ROSAT-ESO Flux-Limited X-ray (REFLEX) catalog of galaxy clusters. The REFLEX survey covers 4.24 steradians (34% of the entire sky) below a declination of 2.5 deg and at high Galactic lati
Externí odkaz:
http://arxiv.org/abs/0907.5457
Autor:
Solovyeva, L., Anokhin, S., Feretti, L., Sauvageot, J. L., Teyssier, R., Giovannini, G., Govoni, F., Neumann, D.
We present a detailed study of the X-ray properties of the galaxy cluster Abell 548b (z=0.04), using XMM-Newton data, and discuss the connection between the thermal properties and the presence of two extended relic radio sources located at the cluste
Externí odkaz:
http://arxiv.org/abs/0804.3607
To study the mass distribution of galaxy clusters up to their Virial radius, CL0016+16 seems to be a good candidate,since it is a bright massive cluster, previously considered as being dynamically relaxed. Using XMM-Newton observations of CL0016+16,
Externí odkaz:
http://arxiv.org/abs/0709.4560
Autor:
Neumann, D. M.
(Abridged) We present in this paper a sample of 14 nearby clusters of galaxies observed with the ROSAT/PSPC. We only select clusters with low galactic nH in order to trace the X-ray emitting intra-cluster medium (ICM) out to large radii. We convert t
Externí odkaz:
http://arxiv.org/abs/astro-ph/0505049
Publikováno v:
Astrophys.J. 625 (2005) 748-753
A previous analysis of the Chandra X-ray image of the center of the cooling core cluster Abell 2597 showed two ``ghost holes'' in the X-ray emission to the west and northeast of the central radio galaxy PKS 2322-123. Previous radio observations did n
Externí odkaz:
http://arxiv.org/abs/astro-ph/0503274
Autor:
Neumann, D. M., Majerowicz, S.
Clusters of galaxies contain a hot gas, which emits in X-rays. X-ray telescopes such as XMM-Newton allow to study this plasma to obtain information on physical quantities of these objects. We present here some results on the total mass density distri
Externí odkaz:
http://arxiv.org/abs/astro-ph/0407601