Soft X-Ray and Extreme Ultraviolet Excess Emission from Clusters of Galaxies
Abstract An excess over the extrapolation to the extreme ultraviolet and soft X-ray ranges of the thermal emission from the hot intracluster medium has been detected in a number of clusters of galaxies. We briefly present each of the satellites (EUVE, ROSAT PSPC and BeppoSAX, and presently XMM-Newto...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Durret, F. [verfasserIn] |
|---|
| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2008 |
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| Schlagwörter: |
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| Anmerkung: |
© Springer Science+Business Media B.V. 2008 |
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| Übergeordnetes Werk: |
Enthalten in: Space science reviews - Springer Netherlands, 1962, 134(2008), 1-4 vom: Feb., Seite 51-70 |
|---|---|
| Übergeordnetes Werk: |
volume:134 ; year:2008 ; number:1-4 ; month:02 ; pages:51-70 |
| Links: |
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| DOI / URN: |
10.1007/s11214-008-9313-8 |
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OLC203369352X |
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| 520 | |a Abstract An excess over the extrapolation to the extreme ultraviolet and soft X-ray ranges of the thermal emission from the hot intracluster medium has been detected in a number of clusters of galaxies. We briefly present each of the satellites (EUVE, ROSAT PSPC and BeppoSAX, and presently XMM-Newton, Chandra and Suzaku) and their corresponding instrumental issues, which are responsible for the fact that this soft excess remains controversial in a number of cases. We then review the evidence for this soft X-ray excess and discuss the possible mechanisms (thermal and non-thermal) which could be responsible for this emission. | ||
| 650 | 4 | |a Galaxies: clusters | |
| 650 | 4 | |a X-ray: spectra | |
| 700 | 1 | |a Kaastra, J. S. |4 aut | |
| 700 | 1 | |a Nevalainen, J. |4 aut | |
| 700 | 1 | |a Ohashi, T. |4 aut | |
| 700 | 1 | |a Werner, N. |4 aut | |
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Soft X-Ray and Extreme Ultraviolet Excess Emission from Clusters of Galaxies |
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Abstract An excess over the extrapolation to the extreme ultraviolet and soft X-ray ranges of the thermal emission from the hot intracluster medium has been detected in a number of clusters of galaxies. We briefly present each of the satellites (EUVE, ROSAT PSPC and BeppoSAX, and presently XMM-Newton, Chandra and Suzaku) and their corresponding instrumental issues, which are responsible for the fact that this soft excess remains controversial in a number of cases. We then review the evidence for this soft X-ray excess and discuss the possible mechanisms (thermal and non-thermal) which could be responsible for this emission. © Springer Science+Business Media B.V. 2008 |
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Abstract An excess over the extrapolation to the extreme ultraviolet and soft X-ray ranges of the thermal emission from the hot intracluster medium has been detected in a number of clusters of galaxies. We briefly present each of the satellites (EUVE, ROSAT PSPC and BeppoSAX, and presently XMM-Newton, Chandra and Suzaku) and their corresponding instrumental issues, which are responsible for the fact that this soft excess remains controversial in a number of cases. We then review the evidence for this soft X-ray excess and discuss the possible mechanisms (thermal and non-thermal) which could be responsible for this emission. © Springer Science+Business Media B.V. 2008 |
| abstract_unstemmed |
Abstract An excess over the extrapolation to the extreme ultraviolet and soft X-ray ranges of the thermal emission from the hot intracluster medium has been detected in a number of clusters of galaxies. We briefly present each of the satellites (EUVE, ROSAT PSPC and BeppoSAX, and presently XMM-Newton, Chandra and Suzaku) and their corresponding instrumental issues, which are responsible for the fact that this soft excess remains controversial in a number of cases. We then review the evidence for this soft X-ray excess and discuss the possible mechanisms (thermal and non-thermal) which could be responsible for this emission. © Springer Science+Business Media B.V. 2008 |
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Soft X-Ray and Extreme Ultraviolet Excess Emission from Clusters of Galaxies |
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Kaastra, J. S. Nevalainen, J. Ohashi, T. Werner, N. |
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