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相关论文: Chandra X-ray observations of Abell 1835 to the vi…

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We present a detailed spectral and spatial analysis of the galaxy cluster PKS 0745-191, using recent observations from the Chandra X-ray Observatory. The data provide information on the temperature and metallicity of the intracluster…

天体物理学 · 物理学 2016-08-30 Amalia K. Hicks , Michael W. Wise , John C. Houck , Claude R. Canizares

We use archival Chandra X-ray Observatory data to investigate X-ray emission from early-type galaxies in the rich z=0.06 cluster Abell 3128. By combining the X-ray count-rates from an input list of optically-selected galaxies, we obtain a…

天体物理学 · 物理学 2009-11-10 Russell J. Smith

We report the detection of the lens cluster of the gravitational lens (GL) system Q0957+561 from a deep observation with the Advanced CCD Imaging Spectrometer on-board the Chandra X-ray Observatory. Intracluster X-ray emission is found to…

天体物理学 · 物理学 2009-11-07 G. Chartas , V. Gupta , G. Garmire , C. Jones , E. E. Falco , I. I. Shapiro , F. Tavecchio

The analysis of a deep (579 ks) Chandra ACIS pointing of the elliptical galaxy NGC4278, which hosts a low luminosity AGN and compact radio emission, allowed us to detect extended emission from hot gas out to a radius of \sim 5 kpc, with a…

高能天体物理现象 · 物理学 2015-06-05 S. Pellegrini , J. Wang , G. Fabbiano , D. W. Kim , N. J. Brassington , J. S. Gallagher , G. Trinchieri , A. Zezas

We present temperature and metallicity maps of the Perseus cluster core obtained with the Chandra X-ray Observatory. We find an overall temperature rise from ~3.0 keV in the core to ~5.5 keV at 120 kpc and a metallicity profile that rises…

天体物理学 · 物理学 2009-09-17 R. W. Schmidt , A. C. Fabian , J. S. Sanders

We report the detection of diffuse hot gas in M31, using archival Chandra observations which allow us to map out a 30' by 30' field (covering a galactocentric radius up to 4.5 kpc) and to detect sources in the galaxy down to a 0.5-8 keV…

天体物理学 · 物理学 2009-11-13 Z. Li , Q. D. Wang

We present Chandra observations of the X-ray environment of a sample of 6 BL Lacertae objects. The improved sensitivity of the ACIS experiment allows us to separate the core X-ray emission from the contribution of diffuse emission from the…

天体物理学 · 物理学 2009-11-07 D. Donato , M. Gliozzi , R. M. Sambruna , J. E. Pesce

We examine deep Chandra X-ray observations of the Centaurus cluster of galaxies, Abell 3526. Applying a gradient magnitude filter reveals a wealth of structure, from filamentary soft emission on 100pc (0.5 arcsec) scales close to the…

We present the results of interferometric observations of the cool core of Abell 1795 at CO(1-0) using the Combined Array for Research in Millimeter-Wave Astronomy. In agreement with previous work, we detect a significant amount of cold…

高能天体物理现象 · 物理学 2015-06-05 Michael McDonald , Lisa H. Wei , Sylvain Veilleux

Abell~1142 is a low-mass galaxy cluster at low redshift containing two comparable Brightest Cluster Galaxies (BCG) resembling a scaled-down version of the Coma Cluster. Our Chandra analysis reveals an X-ray emission peak, roughly 100 kpc…

高能天体物理现象 · 物理学 2016-04-20 Yuanyuan Su , David A. Buote , Fabio Gastaldello , Reinout van Weeren

We present results from the combination of two Chandra pointings of the central region of the cluster of galaxies A3667. From the data analysis of the first pointing Vikhlinin et al. reported the discovery of a prominent cold front which is…

天体物理学 · 物理学 2009-11-07 Pasquale Mazzotta , Roberto Fusco-Femiano , Alexey Vikhlinin

We study the properties of hot gaseous halos in 10 nearby ultraluminous IRAS galaxies observed with the ACIS instrument on board Chandra. For all sample galaxies, diffuse soft X-ray emissions are found within ~10 kpc of the central region;…

天体物理学 · 物理学 2008-11-26 Z. Y. Huo , X. Y. Xia , S. J. Xue , S. Mao , Z. G. Deng

We present a Chandra observation of the cooling flow cluster Abell 262. Spectral fits show that the intracluster medium (ICM) in A262 cools by a factor of three from 2.7 keV to 0.9 keV at the cluster center. A mass deposition rate of Mdot =…

天体物理学 · 物理学 2009-11-10 Elizabeth L. Blanton , Craig L. Sarazin , Brian R. McNamara , T. E. Clarke

Terzan 5, a globular cluster (GC) prominent in mass and population of compact objects, is searched for diffuse X-ray emission, as proposed by several models. We analyzed the data of an archival Chandra observation of Terzan 5 to search for…

高能天体物理现象 · 物理学 2015-05-18 P. Eger , W. Domainko , A. -C. Clapson

Using new XMM and Chandra observations we present an analysis of the temperature structure of the hot gas within a radius of 100 kpc of the bright nearby galaxy group NGC 5044. A spectral deprojection analysis of data extracted from…

天体物理学 · 物理学 2009-11-07 David A. Buote , Aaron D. Lewis , Fabrizio Brighenti , William G. Mathews

We report here the results of the first Chandra X-Ray Observatory observations of the globular cluster M28 (NGC 6626). 46 X-ray sources are detected, of which 12 lie within one core radius of the center. We show that the apparently extended…

We present Suzaku observations of the galaxy cluster Abell 2029, which exploit Suzaku's low particle background to probe the ICM to radii beyond those possible with previous observations (reaching out to the virial radius), and with better…

宇宙学与河外天体物理 · 物理学 2015-06-04 S. A. Walker , A. C. Fabian , J. S. Sanders , M. R. George , Y. Tawara

The superb spatial resolution of Chandra is utilized to study the X-ray morphology of the dwarf starburst galaxy NGC1800 embedded in a small group of galaxies. Diffuse galactic emission is detected, extending several kpc above the galactic…

天体物理学 · 物理学 2009-11-10 Jesper Rasmussen , Ian R. Stevens , Trevor J. Ponman

We present a combined X-ray and optical analysis of the cold front cluster Abell 1201 using archival Chandra, data and multi-object spectroscopy taken with the 3.9m Anglo Australian and 6.5m Multiple Mirror Telescopes. This paper represents…

天体物理学 · 物理学 2011-02-11 Matt S. Owers , Paul E. J. Nulsen , Warrick J. Couch , Maxim Markevitch , Gregory B. Poole

In high-resolution X-ray observations of the hot plasma in clusters of galaxies significant structures caused by AGN feedback, mergers, and turbulence can be detected. Many clusters have been observed by Chandra in great depth and at high…

宇宙学与河外天体物理 · 物理学 2016-01-13 F. Hofmann , J. S. Sanders , K. Nandra , N. Clerc , M. Gaspari