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相关论文: Suzaku Observations of the cluster of galaxies Abe…

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Context: We present results of Suzaku observations of a nearby galaxy cluster A76 at z=0.0395. This cluster is characterized by extremely low X-ray surface brightness and is hereafter referred to as the LSB cluster. Aims: To understand the…

宇宙学与河外天体物理 · 物理学 2015-06-16 N. Ota , Y. Fujino , Y. Ibaraki , H. Boehringer , G. Chon

The results of Suzaku observations of the outskirts of Abell 3395 including a large-scale structure filament toward Abell 3391 are presented. We measured temperature and abundance distributions from the southern outskirt of Abell 3395 to…

宇宙学与河外天体物理 · 物理学 2017-12-20 Yuuki Sugawara , Motokazu Takizawa , Madoka Itahana , Hiroki Akamatsu , Yutaka Fujita , Takaya Ohashi , Yoshitaka Ishisaki

Clusters of galaxies are among the best candidates for particle acceleration sources in the universe, a signature of which is non-thermal hard X-ray emission from the accelerated relativistic particles. We present early results on Suzaku…

The physics of the coolest phases in the hot Intra-Cluster Medium (ICM) of clusters of galaxies is yet to be fully unveiled. X-ray cavities blown by the central Active Galactic Nucleus (AGN) contain enough energy to heat the surrounding gas…

宇宙学与河外天体物理 · 物理学 2011-05-25 J. de Plaa , N. Werner , A. Simionescu , J. S. Kaastra , Y. G. Grange , Jacco Vink

We have analyzed ASCA and ROSAT PSPC spectra and images of the galaxy cluster Abell 2029. The ASCA spectra of the cluster indicate that the gas temperature declines with radius. The PSPC image shows that the cluster is very regular and…

天体物理学 · 物理学 2009-10-30 Craig L. Sarazin , Michael W. Wise , Maxim L. Markevitch

The thermodynamic properties of the intracluster medium (ICM) at the outskirts of galaxy clusters provide valuable insights into the growth of the dark matter halo and the heating of the ICM. Considering the results of the soft X-ray…

We present an analysis of the Chandra X-ray observation of Abell 2052, including large scale properties of the cluster as well as the central region which includes the bright radio source, 3C 317. We present temperature and abundance…

天体物理学 · 物理学 2011-07-18 Elizabeth L. Blanton , Craig L. Sarazin , Brian R. McNamara

We present results from a BeppoSAX observation of the rich cluster Abell 2319. The broad band spectrum (2-50 keV) of the cluster can be adequately represented by an optically thin thermal emission model with a temperature of 9.6+/-0.3 keV…

天体物理学 · 物理学 2009-10-31 S. Molendi , S. De Grandi , R. Fusco-Femiano , S. Colafrancesco , F. Fiore , R. Nesci , F. Tamburelli

We carried out 3 observations of the cluster of galaxies AWM 7, for the central region and 20'-east and 20'-west offset regions, with Suzaku. Temperature and abundance profiles are measured out to 27'~ 570 /h_70 kpc, which corresponded to…

We present results of 120 ks observation of a compact group of galaxies HCG~62 ($z=0.0145$) with Suzaku XIS and HXD-PIN\@. The XIS spectra for four annular regions were fitted with two temperature {\it vapec} model with variable abundance,…

We report properties of the intracluster medium (ICM) in Abell~1246 to the virial radius ($r_{200}$) and further outside as observed with Suzaku. The ICM emission is clearly detected to $r_{200}$, and we derive profiles of electron…

宇宙学与河外天体物理 · 物理学 2015-06-19 K. Sato , K. Matsushita , N. Y. Yamasaki , S. Sasaki , T. Ohashi

We present the results of deep 140 ks Suzaku X-ray observations of the north-east (NE) radio relic of the merging galaxy cluster Abell2255. The temperature structure of Abell2255 is measured out to 0.9 times the virial radius (1.9 Mpc) in…

Previous X-ray and optical studies of the galaxy cluster pair Abell 222/223 suggested the possible presence of a filamentary structure connecting the two clusters, a result that appears to be supported by subsequent weak-lensing analyses.…

宇宙学与河外天体物理 · 物理学 2025-06-03 Yanling Chen , Wei Cui , Aurora Simionescu , Rui Huang , Dan Hu

We present results from a BeppoSAX observation of the rich cluster Abell 3266. The broad band spectrum (2-50 keV) of the cluster, when fitted with an optically thin thermal emission model, yields a temperature of 8.1 +/- 0.2 keV and a metal…

天体物理学 · 物理学 2009-10-31 Sabrina De Grandi , Silvano Molendi

Wide-band Suzaku data on the merging cluster Abell 3667 were examined for hard X-ray emission in excess to the known thermal component. Suzaku detected X-ray signals in the wide energy band from 0.5 to 40 keV. The hard X-ray (> 10 keV) flux…

The thermal, chemical, and kinematic properties of the potentially multi-phase circum/inter-galactic medium at the virial radii of galaxy clusters remain largely uncertain. We present an X-ray study of Abell 2246 and GMBCG…

高能天体物理现象 · 物理学 2015-06-18 Q. Daniel Wang , Stephen Walker

We observed an extended X-ray source designated as Suzaku J1759-3450 with the Suzaku and Chandra observations towards 1RXS J175911.0-344921, which is an unidentified X-ray source listed in the ROSAT Bright Source Catalogue. A conspicuous…

高能天体物理现象 · 物理学 2015-06-16 Hideyuki Mori , Yoshitomo Maeda , Akihiro Furuzawa , Yoshito Haba , Yoshihiro Ueda

We report on the abundance of metals (Mg and Fe) in the intracluster medium (ICM) at the outskirts (0.2 r200 - 0.8 r200) of the Perseus cluster. The X-ray spectra were obtained in the Suzaku/XIS mapping observations of this region. We…

宇宙学与河外天体物理 · 物理学 2015-06-12 S. Ueda , K. Hayashida , H. Nakajima , H. Tsunemi

We present a joint Suzaku and XMM-Newton analysis of the outskirts of the nearby galaxy cluster Abell 2199, the only nearby galaxy cluster to be observed with near complete azimuthal coverage with Suzaku. Using the XMM-Newton observations…

宇宙学与河外天体物理 · 物理学 2020-08-05 M. S. Mirakhor , S. A. Walker

We present the results from Suzaku observations of the Perseus galaxy cluster, which is relatively close, the brightest in the X-ray sky and a relaxed object with a cool core. A number of exposures of central regions and offset pointing…

宇宙学与河外天体物理 · 物理学 2015-06-18 Takayuki Tamura , N. Yamasaki , R. Iizuka , Y. Fukazawa , K. Hayashida , S. Ueda , K. Matsushita , K. Sato , K. Nakazawa , N. Ota , M. Takizawa