ASTRO-H White Paper - Clusters of Galaxies and Related Science
Abstrak
The next generation X-ray observatory ASTRO-H will open up a new dimension in the study of galaxy clusters by achieving for the first time the spectral resolution required to measure velocities of the intracluster plasma, and extending at the same time the spectral coverage to energies well beyond 10 keV. This white paper provides an overview of the capabilities of ASTRO-H for exploring gas motions in galaxy clusters including their cosmological implications, the physics of AGN feedback, dynamics of cluster mergers as well as associated high-energy processes, chemical enrichment of the intracluster medium, and the nature of missing baryons and unidentified dark matter.
Topik & Kata Kunci
Penulis (40)
Rich Kelley
F. Aharonian
Hiroki Akamatsu
F. Akimoto
Steve Allen
N. Anabuki
L. Angelini
Keith Arnaud
M. Audard
H. Awaki
R. Blandford
G. Brown
E. Cackett
E. Costantini
T. Dotani
K. Ebisawa
M. Eckart
T. Enoto
Y. Ezoe
A. Fabian
C. Ferrigno
R. Fujimoto
A. Furuzawa
P. Gandhi
M. Guainazzi
Y. Haba
Kenji Hamaguchi
T. Hayashi
Katsuhiro Hayashi
Y. Inoue
K. Ishibashi
M. Ishida
Y. Ishisaki
J. Kaastra
T. Kallman
T. Kamae
S. Katsuda
M. Kawaharada
D. Khangulyan
C. Kilbourne
Akses Cepat
PDF tidak tersedia langsung
Cek di sumber asli →- Tahun Terbit
- 2014
- Bahasa
- en
- Total Sitasi
- 31×
- Sumber Database
- Semantic Scholar
- Akses
- Open Access ✓