TY - JOUR
T1 - Clusters of galaxies
T2 - Beyond the thermal view
AU - Kaastra, J. S.
AU - Bykov, A. M.
AU - Schindler, S.
AU - Bleeker, J. A.M.
AU - Borgani, S.
AU - Diaferio, A.
AU - Dolag, K.
AU - Durret, F.
AU - Nevalainen, J.
AU - Ohashi, T.
AU - Paerels, F. B.S.
AU - Petrosian, V.
AU - Rephaeli, Y.
AU - Richter, P.
AU - Schaye, J.
AU - Werner, N.
N1 - Funding Information:
Acknowledgements The authors thank ISSI (Bern) for support of the team “Non-virialized X-ray components in clusters of galaxies”. SRON is supported financially by NWO, the Netherlands Organization for Scientific Research. A.M.B. acknowledges the RBRF grant 06-02-16844, a support from RAS Presidium Programs, and a support from NASA ATP (NNX07AG79G). S.S. acknowledges financial support by the Austrian Science Foundation (FWF) through grants P18523-N16 and P19300-N16, by the Tiroler Wissenschaftsfonds and through the UniInfrastrukturprogramm 2005/06 by the BMWF. A.D. gratefully acknowledges support from the PRIN2006 grant “Costituenti fondamentali dell’Universo” of the Italian Ministry of University and Scientific Research and from the INFN grant PD51. F.D. acknowledges support from CNES. J.N. acknowledges support from the Academy of Finland. F.P. acknowledges support from the Dutch Organization for Scientific Research NWO. N.W. acknowledges support by the Marie Curie EARA Early Stage Training visiting fellowship.
PY - 2008/2
Y1 - 2008/2
N2 - We present the work of an international team at the International Space Science Institute (ISSI) in Bern that worked together to review the current observational and theoretical status of the non-virialised X-ray emission components in clusters of galaxies. The subject is important for the study of large-scale hierarchical structure formation and to shed light on the "missing baryon" problem. The topics of the team work include thermal emission and absorption from the warm-hot intergalactic medium, non-thermal X-ray emission in clusters of galaxies, physical processes and chemical enrichment of this medium and clusters of galaxies, and the relationship between all these processes. One of the main goals of the team is to write and discuss a series of review papers on this subject. These reviews are intended as introductory text and reference for scientists wishing to work actively in this field. The team consists of sixteen experts in observations, theory and numerical simulations.
AB - We present the work of an international team at the International Space Science Institute (ISSI) in Bern that worked together to review the current observational and theoretical status of the non-virialised X-ray emission components in clusters of galaxies. The subject is important for the study of large-scale hierarchical structure formation and to shed light on the "missing baryon" problem. The topics of the team work include thermal emission and absorption from the warm-hot intergalactic medium, non-thermal X-ray emission in clusters of galaxies, physical processes and chemical enrichment of this medium and clusters of galaxies, and the relationship between all these processes. One of the main goals of the team is to write and discuss a series of review papers on this subject. These reviews are intended as introductory text and reference for scientists wishing to work actively in this field. The team consists of sixteen experts in observations, theory and numerical simulations.
KW - Galaxies: clusters: general
KW - Intergalactic medium
KW - Large-scale structure of universe
KW - X-rays: galaxy clusters
UR - http://www.scopus.com/inward/record.url?scp=39049146999&partnerID=8YFLogxK
U2 - 10.1007/s11214-008-9326-3
DO - 10.1007/s11214-008-9326-3
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AN - SCOPUS:39049146999
SN - 0038-6308
VL - 134
SP - 1
EP - 6
JO - Space Science Reviews
JF - Space Science Reviews
IS - 1-4
ER -