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Soft X-Ray and Extreme Ultraviolet Excess Emission from Clusters of Galaxies
- Source :
- Space Science Reviews. 134(1-4):51-70
- Publisher :
- Springer Nature
-
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.<br />21 pages, 5 figures, accepted for publication in Space Science Reviews, special issue "Clusters of galaxies: beyond the thermal view", Editor J.S. Kaastra, Chapter 4; work done by an international team at the International Space Science Institute (ISSI), Bern, organised by J.S. Kaastra, A.M.Bykov, S. Schindler & J.A.M. Bleeker
- Subjects :
- Physics
Soft x ray
010308 nuclear & particles physics
Astrophysics::High Energy Astrophysical Phenomena
Astrophysics (astro-ph)
Extrapolation
FOS: Physical sciences
Astronomy and Astrophysics
Thermal emission
Astrophysics
Astrophysics::Cosmology and Extragalactic Astrophysics
01 natural sciences
Galaxy
Space and Planetary Science
Extreme ultraviolet
Intracluster medium
0103 physical sciences
ROSAT
Thermal
010303 astronomy & astrophysics
Subjects
Details
- Language :
- English
- ISSN :
- 00386308
- Volume :
- 134
- Issue :
- 1-4
- Database :
- OpenAIRE
- Journal :
- Space Science Reviews
- Accession number :
- edsair.doi.dedup.....7c80fed0a58bb657a36d1d95b27e88c1
- Full Text :
- https://doi.org/10.1007/s11214-008-9313-8