「すざく」，宇宙で最重量級の衝突現場を検証する

- my web page
- ISAStopics
- ustrem
- ISAS News 2012-02, すざく」で探る銀河団プラズマの運動

「すざく」衛星による銀河団の外側のICMの観測

日本天文学会2006年春季年会

宇宙学校・とうきょう 〜宇宙に夢中！〜

講師として参加しました。

http://www.isas.jaxa.jp/j/topics/event/2011/1103_tokyo.shtml

世界の最先端を切り拓く日本のX線天文学　ー「すざく」からASTRO-Hへ

Workshop on Chemical Evolution of the Universe

http://www-x.phys.se.tmu.ac.jp/ceu11/Top.html

科研費 申請

Sterile neutrinos

Nature, 2011, Oct
http://www.nature.com/nature/journal/v478/n7369/full/478328a.html

Nature

 

478,

 

328–329

 

(20 October 2011)

 

doi:10.1038/478328a

WILLIAM C. LOUIS

高宇連 第11回研究会 @ 早稲田

http://heapa.astro.isas.jaxa.jp/activity/2011/heapaws11/

水説:原発ゼロが世論か＝潮田道夫

潮田道夫氏の意見は参考になる。
暮しの手帖のエッセイを読んでいる。

http://mainichi.jp/opinion/news/20120808ddm003070095000c.html

毎日新聞　2012年08月08日　東京朝刊

Suzaku conference @ SLAC 2011-7

2011-7-20-22 @ SLAC
http://www.confcon.com/suzaku2011/

- 2011-05-25
submitted abstract.

Structure in Clusters and Groups of Galaxies in the Chandra Era 2011, July

2011-7-11-14, @ Bonston, MA
http://cxc.harvard.edu/cdo/xclust11/

suzaku @ USC 2011-4

2011/4/2-4/12

IXO meeting, Rome, 2011-3

http://www.iasf-roma.inaf.it/IXO/
I presented
Suzaku measurements of gas bulk motions in galaxy clusters.
The presentation pdf can be found below.
http://www.iasf-roma.inaf.it/IXO/IXOProgramme.htm

High-Energy Radiation in Galactic Compact Sources, Valenti Bosch-Ramon

SEMINAR DATE: Feb 10 (Thursday)
TIME: 17:00 h
SPEAKER: Dr. Valenti Bosch-Ramon
AFFILIATION: DIAS, Dublin, Ireland

SEMINAR TITLE: High-Energy Radiation in Galactic Compact Sources
SEMINAR LANGUAGE: English

ABSTRACT:
Galactic compact sources have been considered a potential class of  
gamma-ray emitting objects for many years, but it was not until  
recently that it was firmly established by satellite-borne GeV and  
ground-based TeV instruments. These sources, basically all of them  
pertaining to the category of gamma-ray binaries, can be very  
luminous, and present strong variability and high acceleration  
efficiencies, being their high-energy emission likely produced in  
powerful outflows suffering internal and external shocks. Since they  
are compact objects and strong radiation fields tend to be present,  
pair creation cannot be neglected. In this talk, I will briefly  
summarize the main properties of these objects, as well as discuss  
open questions regarding the physics behind their emission.

Komatsu et al. 2011, WMAP 7year

http://adsabs.harvard.edu/abs/2011ApJS..192...18K

Discovery of Gas Bulk Motion in the Galaxy Cluster Abell 2256 with Suzaku

2011-1-31
submitted to PASJ.

2011-03-28
accepted.
This is my 10th 1st-author paper.

http://adsabs.harvard.edu/abs/2011PASJ...63S1009T


In ISAS news in 2012 -
http://www.isas.jaxa.jp/e/forefront/2012/tamura/

Nature articles by A.C. Fabian

http://bit.ly/dN1Hj0