Structures and Components in Galaxy Clusters: Observations and Models
Abstract Clusters of galaxies are the largest gravitationally bounded structures in the Universe dominated by dark matter. We review the observational appearance and physical models of plasma structures in clusters of galaxies. Bubbles of relativistic plasma which are inflated by supermassive black...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Bykov, A. M. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2015 |
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| Schlagwörter: |
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| Anmerkung: |
© Springer Science+Business Media Dordrecht 2015 |
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| Übergeordnetes Werk: |
Enthalten in: Space science reviews - Springer Netherlands, 1962, 188(2015), 1-4 vom: 04. Feb., Seite 141-185 |
|---|---|
| Übergeordnetes Werk: |
volume:188 ; year:2015 ; number:1-4 ; day:04 ; month:02 ; pages:141-185 |
| Links: |
|---|
| DOI / URN: |
10.1007/s11214-014-0129-4 |
|---|
| Katalog-ID: |
OLC2033701158 |
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| 520 | |a Abstract Clusters of galaxies are the largest gravitationally bounded structures in the Universe dominated by dark matter. We review the observational appearance and physical models of plasma structures in clusters of galaxies. Bubbles of relativistic plasma which are inflated by supermassive black holes of AGNs, cooling and heating of the gas, large scale plasma shocks, cold fronts, non-thermal halos and relics are observed in clusters. These constituents are reflecting both the formation history and the dynamical properties of clusters of galaxies. We discuss X-ray spectroscopy as a tool to study the metal enrichment in clusters and fine spectroscopy of Fe X-ray lines as a powerful diagnostics of both the turbulent plasma motions and the energetics of the non-thermal electron populations. The knowledge of the complex dynamical and feedback processes is necessary to understand the energy and matter balance as well as to constrain the role of the non-thermal components of clusters. | ||
| 650 | 4 | |a Clusters of galaxies | |
| 650 | 4 | |a Radiation mechanisms: non-thermal | |
| 650 | 4 | |a Radio continuum | |
| 650 | 4 | |a X-rays: galaxies: clusters | |
| 700 | 1 | |a Churazov, E. M. |4 aut | |
| 700 | 1 | |a Ferrari, C. |4 aut | |
| 700 | 1 | |a Forman, W. R. |4 aut | |
| 700 | 1 | |a Kaastra, J. S. |4 aut | |
| 700 | 1 | |a Klein, U. |4 aut | |
| 700 | 1 | |a Markevitch, M. |4 aut | |
| 700 | 1 | |a de Plaa, J. |4 aut | |
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10.1007/s11214-014-0129-4 doi (DE-627)OLC2033701158 (DE-He213)s11214-014-0129-4-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Bykov, A. M. verfasserin aut Structures and Components in Galaxy Clusters: Observations and Models 2015 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2015 Abstract Clusters of galaxies are the largest gravitationally bounded structures in the Universe dominated by dark matter. We review the observational appearance and physical models of plasma structures in clusters of galaxies. Bubbles of relativistic plasma which are inflated by supermassive black holes of AGNs, cooling and heating of the gas, large scale plasma shocks, cold fronts, non-thermal halos and relics are observed in clusters. These constituents are reflecting both the formation history and the dynamical properties of clusters of galaxies. We discuss X-ray spectroscopy as a tool to study the metal enrichment in clusters and fine spectroscopy of Fe X-ray lines as a powerful diagnostics of both the turbulent plasma motions and the energetics of the non-thermal electron populations. The knowledge of the complex dynamical and feedback processes is necessary to understand the energy and matter balance as well as to constrain the role of the non-thermal components of clusters. Clusters of galaxies Radiation mechanisms: non-thermal Radio continuum X-rays: galaxies: clusters Churazov, E. M. aut Ferrari, C. aut Forman, W. R. aut Kaastra, J. S. aut Klein, U. aut Markevitch, M. aut de Plaa, J. aut Enthalten in Space science reviews Springer Netherlands, 1962 188(2015), 1-4 vom: 04. Feb., Seite 141-185 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:188 year:2015 number:1-4 day:04 month:02 pages:141-185 https://doi.org/10.1007/s11214-014-0129-4 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_22 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4306 GBV_ILN_4700 AR 188 2015 1-4 04 02 141-185 |
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10.1007/s11214-014-0129-4 doi (DE-627)OLC2033701158 (DE-He213)s11214-014-0129-4-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Bykov, A. M. verfasserin aut Structures and Components in Galaxy Clusters: Observations and Models 2015 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2015 Abstract Clusters of galaxies are the largest gravitationally bounded structures in the Universe dominated by dark matter. We review the observational appearance and physical models of plasma structures in clusters of galaxies. Bubbles of relativistic plasma which are inflated by supermassive black holes of AGNs, cooling and heating of the gas, large scale plasma shocks, cold fronts, non-thermal halos and relics are observed in clusters. These constituents are reflecting both the formation history and the dynamical properties of clusters of galaxies. We discuss X-ray spectroscopy as a tool to study the metal enrichment in clusters and fine spectroscopy of Fe X-ray lines as a powerful diagnostics of both the turbulent plasma motions and the energetics of the non-thermal electron populations. The knowledge of the complex dynamical and feedback processes is necessary to understand the energy and matter balance as well as to constrain the role of the non-thermal components of clusters. Clusters of galaxies Radiation mechanisms: non-thermal Radio continuum X-rays: galaxies: clusters Churazov, E. M. aut Ferrari, C. aut Forman, W. R. aut Kaastra, J. S. aut Klein, U. aut Markevitch, M. aut de Plaa, J. aut Enthalten in Space science reviews Springer Netherlands, 1962 188(2015), 1-4 vom: 04. Feb., Seite 141-185 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:188 year:2015 number:1-4 day:04 month:02 pages:141-185 https://doi.org/10.1007/s11214-014-0129-4 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_22 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4306 GBV_ILN_4700 AR 188 2015 1-4 04 02 141-185 |
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10.1007/s11214-014-0129-4 doi (DE-627)OLC2033701158 (DE-He213)s11214-014-0129-4-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Bykov, A. M. verfasserin aut Structures and Components in Galaxy Clusters: Observations and Models 2015 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2015 Abstract Clusters of galaxies are the largest gravitationally bounded structures in the Universe dominated by dark matter. We review the observational appearance and physical models of plasma structures in clusters of galaxies. Bubbles of relativistic plasma which are inflated by supermassive black holes of AGNs, cooling and heating of the gas, large scale plasma shocks, cold fronts, non-thermal halos and relics are observed in clusters. These constituents are reflecting both the formation history and the dynamical properties of clusters of galaxies. We discuss X-ray spectroscopy as a tool to study the metal enrichment in clusters and fine spectroscopy of Fe X-ray lines as a powerful diagnostics of both the turbulent plasma motions and the energetics of the non-thermal electron populations. The knowledge of the complex dynamical and feedback processes is necessary to understand the energy and matter balance as well as to constrain the role of the non-thermal components of clusters. Clusters of galaxies Radiation mechanisms: non-thermal Radio continuum X-rays: galaxies: clusters Churazov, E. M. aut Ferrari, C. aut Forman, W. R. aut Kaastra, J. S. aut Klein, U. aut Markevitch, M. aut de Plaa, J. aut Enthalten in Space science reviews Springer Netherlands, 1962 188(2015), 1-4 vom: 04. Feb., Seite 141-185 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:188 year:2015 number:1-4 day:04 month:02 pages:141-185 https://doi.org/10.1007/s11214-014-0129-4 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_22 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4306 GBV_ILN_4700 AR 188 2015 1-4 04 02 141-185 |
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10.1007/s11214-014-0129-4 doi (DE-627)OLC2033701158 (DE-He213)s11214-014-0129-4-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Bykov, A. M. verfasserin aut Structures and Components in Galaxy Clusters: Observations and Models 2015 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2015 Abstract Clusters of galaxies are the largest gravitationally bounded structures in the Universe dominated by dark matter. We review the observational appearance and physical models of plasma structures in clusters of galaxies. Bubbles of relativistic plasma which are inflated by supermassive black holes of AGNs, cooling and heating of the gas, large scale plasma shocks, cold fronts, non-thermal halos and relics are observed in clusters. These constituents are reflecting both the formation history and the dynamical properties of clusters of galaxies. We discuss X-ray spectroscopy as a tool to study the metal enrichment in clusters and fine spectroscopy of Fe X-ray lines as a powerful diagnostics of both the turbulent plasma motions and the energetics of the non-thermal electron populations. The knowledge of the complex dynamical and feedback processes is necessary to understand the energy and matter balance as well as to constrain the role of the non-thermal components of clusters. Clusters of galaxies Radiation mechanisms: non-thermal Radio continuum X-rays: galaxies: clusters Churazov, E. M. aut Ferrari, C. aut Forman, W. R. aut Kaastra, J. S. aut Klein, U. aut Markevitch, M. aut de Plaa, J. aut Enthalten in Space science reviews Springer Netherlands, 1962 188(2015), 1-4 vom: 04. Feb., Seite 141-185 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:188 year:2015 number:1-4 day:04 month:02 pages:141-185 https://doi.org/10.1007/s11214-014-0129-4 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_22 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4306 GBV_ILN_4700 AR 188 2015 1-4 04 02 141-185 |
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10.1007/s11214-014-0129-4 doi (DE-627)OLC2033701158 (DE-He213)s11214-014-0129-4-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Bykov, A. M. verfasserin aut Structures and Components in Galaxy Clusters: Observations and Models 2015 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2015 Abstract Clusters of galaxies are the largest gravitationally bounded structures in the Universe dominated by dark matter. We review the observational appearance and physical models of plasma structures in clusters of galaxies. Bubbles of relativistic plasma which are inflated by supermassive black holes of AGNs, cooling and heating of the gas, large scale plasma shocks, cold fronts, non-thermal halos and relics are observed in clusters. These constituents are reflecting both the formation history and the dynamical properties of clusters of galaxies. We discuss X-ray spectroscopy as a tool to study the metal enrichment in clusters and fine spectroscopy of Fe X-ray lines as a powerful diagnostics of both the turbulent plasma motions and the energetics of the non-thermal electron populations. The knowledge of the complex dynamical and feedback processes is necessary to understand the energy and matter balance as well as to constrain the role of the non-thermal components of clusters. Clusters of galaxies Radiation mechanisms: non-thermal Radio continuum X-rays: galaxies: clusters Churazov, E. M. aut Ferrari, C. aut Forman, W. R. aut Kaastra, J. S. aut Klein, U. aut Markevitch, M. aut de Plaa, J. aut Enthalten in Space science reviews Springer Netherlands, 1962 188(2015), 1-4 vom: 04. Feb., Seite 141-185 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:188 year:2015 number:1-4 day:04 month:02 pages:141-185 https://doi.org/10.1007/s11214-014-0129-4 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_22 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4306 GBV_ILN_4700 AR 188 2015 1-4 04 02 141-185 |
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Bykov, A. M. Churazov, E. M. Ferrari, C. Forman, W. R. Kaastra, J. S. Klein, U. Markevitch, M. de Plaa, J. |
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structures and components in galaxy clusters: observations and models |
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Structures and Components in Galaxy Clusters: Observations and Models |
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Abstract Clusters of galaxies are the largest gravitationally bounded structures in the Universe dominated by dark matter. We review the observational appearance and physical models of plasma structures in clusters of galaxies. Bubbles of relativistic plasma which are inflated by supermassive black holes of AGNs, cooling and heating of the gas, large scale plasma shocks, cold fronts, non-thermal halos and relics are observed in clusters. These constituents are reflecting both the formation history and the dynamical properties of clusters of galaxies. We discuss X-ray spectroscopy as a tool to study the metal enrichment in clusters and fine spectroscopy of Fe X-ray lines as a powerful diagnostics of both the turbulent plasma motions and the energetics of the non-thermal electron populations. The knowledge of the complex dynamical and feedback processes is necessary to understand the energy and matter balance as well as to constrain the role of the non-thermal components of clusters. © Springer Science+Business Media Dordrecht 2015 |
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Abstract Clusters of galaxies are the largest gravitationally bounded structures in the Universe dominated by dark matter. We review the observational appearance and physical models of plasma structures in clusters of galaxies. Bubbles of relativistic plasma which are inflated by supermassive black holes of AGNs, cooling and heating of the gas, large scale plasma shocks, cold fronts, non-thermal halos and relics are observed in clusters. These constituents are reflecting both the formation history and the dynamical properties of clusters of galaxies. We discuss X-ray spectroscopy as a tool to study the metal enrichment in clusters and fine spectroscopy of Fe X-ray lines as a powerful diagnostics of both the turbulent plasma motions and the energetics of the non-thermal electron populations. The knowledge of the complex dynamical and feedback processes is necessary to understand the energy and matter balance as well as to constrain the role of the non-thermal components of clusters. © Springer Science+Business Media Dordrecht 2015 |
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Abstract Clusters of galaxies are the largest gravitationally bounded structures in the Universe dominated by dark matter. We review the observational appearance and physical models of plasma structures in clusters of galaxies. Bubbles of relativistic plasma which are inflated by supermassive black holes of AGNs, cooling and heating of the gas, large scale plasma shocks, cold fronts, non-thermal halos and relics are observed in clusters. These constituents are reflecting both the formation history and the dynamical properties of clusters of galaxies. We discuss X-ray spectroscopy as a tool to study the metal enrichment in clusters and fine spectroscopy of Fe X-ray lines as a powerful diagnostics of both the turbulent plasma motions and the energetics of the non-thermal electron populations. The knowledge of the complex dynamical and feedback processes is necessary to understand the energy and matter balance as well as to constrain the role of the non-thermal components of clusters. © Springer Science+Business Media Dordrecht 2015 |
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Structures and Components in Galaxy Clusters: Observations and Models |
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