http://arxiv.org/abs/1412.1176
2014-12
Kitayama et al.
(2015-01-22)
Collaborated with ASTRO-H SWG, I contributed to this work.
(copy, abstract)
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.
2015年1月22日木曜日
2015年1月17日土曜日
Suzaku Observations of Abell 1795: Cluster Emission to r200
http://adsabs.harvard.edu/abs/2009PASJ...61.1117B
http://pasj.oxfordjournals.org/content/61/5/1117
2015-01-17
One of the most cited Suzaku papers.
Some papers citing this.
http://adsabs.harvard.edu/abs/2011ApJ...738...48A
http://adsabs.harvard.edu/abs/2011ApJ...731L..10N
http://adsabs.harvard.edu/abs/2011MNRAS.414.2101U
http://adsabs.harvard.edu/abs/2010ApJ...721.1105B
http://adsabs.harvard.edu/abs/2014arXiv1406.4352E
http://pasj.oxfordjournals.org/content/61/5/1117
2015-01-17
One of the most cited Suzaku papers.
Some papers citing this.
http://adsabs.harvard.edu/abs/2011ApJ...738...48A
http://adsabs.harvard.edu/abs/2011ApJ...731L..10N
http://adsabs.harvard.edu/abs/2011MNRAS.414.2101U
http://adsabs.harvard.edu/abs/2010ApJ...721.1105B
http://adsabs.harvard.edu/abs/2014arXiv1406.4352E
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