The Hot and Energetic Universe: The evolution of galaxy groups and clusters

E. Pointecouteau; T. H. Reiprich; C. Adami; M. Arnaud; V. Biffi; S. Borgani; K. Borm; H. Bourdin; M. Brueggen; E. Bulbul; N. Clerc; J. H. Croston; K. Dolag; S. Ettori; A. Finoguenov; J. Kaastra; L. Lovisari; B. Maughan; P. Mazzotta; F. Pacaud; J. de Plaa; G. W. Pratt; M. Ramos-Ceja; E. Rasia; J. Sanders; Y. -Y. Zhang; S. Allen; H. Boehringer; G. Brunetti; D. Elbaz; R. Fassbender; H. Hoekstra; H. Hildebrandt; G. Lamer; D. Marrone; J. Mohr; S. Molendi; J. Nevalainen; T. Ohashi; N. Ota; M. Pierre; K. Romer; S. Schindler; T. Schrabback; A. Schwope; R. Smith; V. Springel; A. von der Linden

The Hot and Energetic Universe: The evolution of galaxy groups and clusters

E. Pointecouteau, T. H. Reiprich, C. Adami, M. Arnaud, V. Biffi, S. Borgani, K. Borm, H. Bourdin, M. Brueggen, E. Bulbul, N. Clerc, J. H. Croston, K. Dolag, S. Ettori, A. Finoguenov, J. Kaastra, L. Lovisari, B. Maughan, P. Mazzotta, F. PacaudJ. de Plaa, G. W. Pratt, M. Ramos-Ceja, E. Rasia, J. Sanders, Y. -Y. Zhang, S. Allen, H. Boehringer, G. Brunetti, D. Elbaz, R. Fassbender, H. Hoekstra, H. Hildebrandt, G. Lamer, D. Marrone, J. Mohr, S. Molendi, J. Nevalainen, T. Ohashi, N. Ota, M. Pierre, K. Romer, S. Schindler, T. Schrabback, A. Schwope, R. Smith, V. Springel, A. von der Linden

School of Physics

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Abstract

Major astrophysical questions related to the formation and evolution of structures, and more specifically of galaxy groups and clusters, will still be open in the coming decade and beyond: what is the interplay of galaxy, supermassive black hole, and intergalactic gas evolution in the most massive objects in the Universe - galaxy groups and clusters? What are the processes driving the evolution of chemical enrichment of the hot diffuse gas in large-scale structures? How and when did the first galaxy groups in the Universe, massive enough to bind more than 10^7 K gas, form? Focussing on the period when groups and clusters assembled (0.5z

Original language	English
Journal	arXiv
Publication status	Published - 10 Jun 2013

Bibliographical note

Supporting paper for the science theme The Hot and Energetic Universe to be implemented by the Athena+ X-ray observatory (http://www.the-athena-x-ray-observatory.eu). 10 pages, 4 figures

Keywords

astro-ph.HE
astro-ph.CO

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Pointecouteau, E. ; H. Reiprich, T. ; Adami, C. ; Arnaud, M. ; Biffi, V. ; Borgani, S. ; Borm, K. ; Bourdin, H. ; Brueggen, M. ; Bulbul, E. ; Clerc, N. ; H. Croston, J. ; Dolag, K. ; Ettori, S. ; Finoguenov, A. ; Kaastra, J. ; Lovisari, L. ; Maughan, B. ; Mazzotta, P. ; Pacaud, F. ; de Plaa, J. ; W. Pratt, G. ; Ramos-Ceja, M. ; Rasia, E. ; Sanders, J. ; -Y. Zhang, Y. ; Allen, S. ; Boehringer, H. ; Brunetti, G. ; Elbaz, D. ; Fassbender, R. ; Hoekstra, H. ; Hildebrandt, H. ; Lamer, G. ; Marrone, D. ; Mohr, J. ; Molendi, S. ; Nevalainen, J. ; Ohashi, T. ; Ota, N. ; Pierre, M. ; Romer, K. ; Schindler, S. ; Schrabback, T. ; Schwope, A. ; Smith, R. ; Springel, V. ; von der Linden, A. / The Hot and Energetic Universe : The evolution of galaxy groups and clusters. In: arXiv. 2013.

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title = "The Hot and Energetic Universe: The evolution of galaxy groups and clusters",

abstract = "Major astrophysical questions related to the formation and evolution of structures, and more specifically of galaxy groups and clusters, will still be open in the coming decade and beyond: what is the interplay of galaxy, supermassive black hole, and intergalactic gas evolution in the most massive objects in the Universe - galaxy groups and clusters? What are the processes driving the evolution of chemical enrichment of the hot diffuse gas in large-scale structures? How and when did the first galaxy groups in the Universe, massive enough to bind more than 10^7 K gas, form? Focussing on the period when groups and clusters assembled (0.5z",

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author = "E. Pointecouteau and {H. Reiprich}, T. and C. Adami and M. Arnaud and V. Biffi and S. Borgani and K. Borm and H. Bourdin and M. Brueggen and E. Bulbul and N. Clerc and {H. Croston}, J. and K. Dolag and S. Ettori and A. Finoguenov and J. Kaastra and L. Lovisari and B. Maughan and P. Mazzotta and F. Pacaud and {de Plaa}, J. and {W. Pratt}, G. and M. Ramos-Ceja and E. Rasia and J. Sanders and {-Y. Zhang}, Y. and S. Allen and H. Boehringer and G. Brunetti and D. Elbaz and R. Fassbender and H. Hoekstra and H. Hildebrandt and G. Lamer and D. Marrone and J. Mohr and S. Molendi and J. Nevalainen and T. Ohashi and N. Ota and M. Pierre and K. Romer and S. Schindler and T. Schrabback and A. Schwope and R. Smith and V. Springel and {von der Linden}, A.",

note = "Supporting paper for the science theme The Hot and Energetic Universe to be implemented by the Athena+ X-ray observatory (http://www.the-athena-x-ray-observatory.eu). 10 pages, 4 figures",

year = "2013",

month = jun,

day = "10",

language = "English",

journal = "arXiv",

publisher = "Cornell University",

}

Pointecouteau, E, H. Reiprich, T, Adami, C, Arnaud, M, Biffi, V, Borgani, S, Borm, K, Bourdin, H, Brueggen, M, Bulbul, E, Clerc, N, H. Croston, J, Dolag, K, Ettori, S, Finoguenov, A, Kaastra, J, Lovisari, L, Maughan, B, Mazzotta, P, Pacaud, F, de Plaa, J, W. Pratt, G, Ramos-Ceja, M, Rasia, E, Sanders, J, -Y. Zhang, Y, Allen, S, Boehringer, H, Brunetti, G, Elbaz, D, Fassbender, R, Hoekstra, H, Hildebrandt, H, Lamer, G, Marrone, D, Mohr, J, Molendi, S, Nevalainen, J, Ohashi, T, Ota, N, Pierre, M, Romer, K, Schindler, S, Schrabback, T, Schwope, A, Smith, R, Springel, V & von der Linden, A 2013, 'The Hot and Energetic Universe: The evolution of galaxy groups and clusters', arXiv.

The Hot and Energetic Universe : The evolution of galaxy groups and clusters. / Pointecouteau, E.; H. Reiprich, T.; Adami, C.; Arnaud, M.; Biffi, V.; Borgani, S.; Borm, K.; Bourdin, H.; Brueggen, M.; Bulbul, E.; Clerc, N.; H. Croston, J.; Dolag, K.; Ettori, S.; Finoguenov, A.; Kaastra, J.; Lovisari, L.; Maughan, B.; Mazzotta, P.; Pacaud, F.; de Plaa, J.; W. Pratt, G.; Ramos-Ceja, M.; Rasia, E.; Sanders, J.; -Y. Zhang, Y.; Allen, S.; Boehringer, H.; Brunetti, G.; Elbaz, D.; Fassbender, R.; Hoekstra, H.; Hildebrandt, H.; Lamer, G.; Marrone, D.; Mohr, J.; Molendi, S.; Nevalainen, J.; Ohashi, T.; Ota, N.; Pierre, M.; Romer, K.; Schindler, S.; Schrabback, T.; Schwope, A.; Smith, R.; Springel, V.; von der Linden, A.

In: arXiv, 10.06.2013.

Research output: Contribution to journal › Article (Academic Journal)

TY - JOUR

T1 - The Hot and Energetic Universe

T2 - The evolution of galaxy groups and clusters

AU - Pointecouteau, E.

AU - H. Reiprich, T.

AU - Adami, C.

AU - Arnaud, M.

AU - Biffi, V.

AU - Borgani, S.

AU - Borm, K.

AU - Bourdin, H.

AU - Brueggen, M.

AU - Bulbul, E.

AU - Clerc, N.

AU - H. Croston, J.

AU - Dolag, K.

AU - Ettori, S.

AU - Finoguenov, A.

AU - Kaastra, J.

AU - Lovisari, L.

AU - Maughan, B.

AU - Mazzotta, P.

AU - Pacaud, F.

AU - de Plaa, J.

AU - W. Pratt, G.

AU - Ramos-Ceja, M.

AU - Rasia, E.

AU - Sanders, J.

AU - -Y. Zhang, Y.

AU - Allen, S.

AU - Boehringer, H.

AU - Brunetti, G.

AU - Elbaz, D.

AU - Fassbender, R.

AU - Hoekstra, H.

AU - Hildebrandt, H.

AU - Lamer, G.

AU - Marrone, D.

AU - Mohr, J.

AU - Molendi, S.

AU - Nevalainen, J.

AU - Ohashi, T.

AU - Ota, N.

AU - Pierre, M.

AU - Romer, K.

AU - Schindler, S.

AU - Schrabback, T.

AU - Schwope, A.

AU - Smith, R.

AU - Springel, V.

AU - von der Linden, A.

N1 - Supporting paper for the science theme The Hot and Energetic Universe to be implemented by the Athena+ X-ray observatory (http://www.the-athena-x-ray-observatory.eu). 10 pages, 4 figures

PY - 2013/6/10

Y1 - 2013/6/10

N2 - Major astrophysical questions related to the formation and evolution of structures, and more specifically of galaxy groups and clusters, will still be open in the coming decade and beyond: what is the interplay of galaxy, supermassive black hole, and intergalactic gas evolution in the most massive objects in the Universe - galaxy groups and clusters? What are the processes driving the evolution of chemical enrichment of the hot diffuse gas in large-scale structures? How and when did the first galaxy groups in the Universe, massive enough to bind more than 10^7 K gas, form? Focussing on the period when groups and clusters assembled (0.5z

AB - Major astrophysical questions related to the formation and evolution of structures, and more specifically of galaxy groups and clusters, will still be open in the coming decade and beyond: what is the interplay of galaxy, supermassive black hole, and intergalactic gas evolution in the most massive objects in the Universe - galaxy groups and clusters? What are the processes driving the evolution of chemical enrichment of the hot diffuse gas in large-scale structures? How and when did the first galaxy groups in the Universe, massive enough to bind more than 10^7 K gas, form? Focussing on the period when groups and clusters assembled (0.5z

KW - astro-ph.HE

KW - astro-ph.CO

M3 - Article (Academic Journal)

JO - arXiv

JF - arXiv

ER -

The Hot and Energetic Universe: The evolution of galaxy groups and clusters

Abstract

Bibliographical note

Keywords

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Research in planetary physics, astrophysics and cosmology at Bristol

Cite this