http://www.nature.com/nature/journal/v507/n7492/full/nature12995.html
2014年3月26日水曜日
2014年3月18日火曜日
First Direct Evidence of Cosmic Inflation
http://www.cfa.harvard.edu/news/2014-05
http://planck.exblog.jp/21835733/
by Ooguri-san
http://nationalgeographic.jp/nng/article/20140328/390221/
by Komatsu-san
2014年3月14日金曜日
X-ray survey of the nearby and relaxed cluster Abell2199
chandra proposal cycle 16
submitted a plan.
ラベル:
Abell2199,
chandra,
suzakuAO10
2014年3月6日木曜日
2014年2月19日水曜日
Suzaku-MAXI 2014
http://wwwxray.ess.sci.osaka-u.ac.jp/SuzakuMAXI2014/
My talk:
X-ray measurements of gas bulk motions in galaxy clusters
X-ray studies of velocity structures of the intracluster medium is one of the primary goals for future X-ray missions. High resolution spectroscopy will provide measurements of energy distributions not only in thermal but also in kinematic forms. These provide understanding of cluster formation and reductions of systematic uncertainties in cluster total masses for precise cosmology. Using Suzaku we have detected a motion of a sub component with a velocity of about 1500 km/s for the first time by X-ray of a X-ray bright merging cluster, Abell2256 (Tamura et al. 2011). We also detected a hint of bulk motion in the Perseus cluster core (Tamura et al. 2013). In addition we attempted to measure 'X-ray gas redshift' of clusters. We found that gas are moving in pair with galaxies at least in X-ray bright central regions. In addition to these new Suzaku results, future studies of gas bulk motion along with turbulent motions by X-ray micro calorimeter onboard ASTRO-H will be discussed.
My talk:
X-ray measurements of gas bulk motions in galaxy clusters
X-ray studies of velocity structures of the intracluster medium is one of the primary goals for future X-ray missions. High resolution spectroscopy will provide measurements of energy distributions not only in thermal but also in kinematic forms. These provide understanding of cluster formation and reductions of systematic uncertainties in cluster total masses for precise cosmology. Using Suzaku we have detected a motion of a sub component with a velocity of about 1500 km/s for the first time by X-ray of a X-ray bright merging cluster, Abell2256 (Tamura et al. 2011). We also detected a hint of bulk motion in the Perseus cluster core (Tamura et al. 2013). In addition we attempted to measure 'X-ray gas redshift' of clusters. We found that gas are moving in pair with galaxies at least in X-ray bright central regions. In addition to these new Suzaku results, future studies of gas bulk motion along with turbulent motions by X-ray micro calorimeter onboard ASTRO-H will be discussed.
ラベル:
a2256,
ehimeU,
In-english,
meeting,
perseus,
popular,
suzaku,
tamura_talk
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