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相关论文: X-ray analysis of Abell 2634 and its central galax…

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We use new ASCA observations and archival ROSAT Position Sensitive Proportional Counter (PSPC) data to determine the X-ray spectral properties of the intracluster gas in Abell 644. From the overall spectrum, we determine the average gas…

天体物理学 · 物理学 2009-10-31 F. E. Bauer , C. L. Sarazin

We present a combined analysis of the BeppoSAX and ROSAT PSPC observation of the cluster of galaxies A3562, a massive member of the core of the Shapley Supercluster. With a complex and interacting structure composed from two groups of…

天体物理学 · 物理学 2016-08-30 S. Ettori , S. Bardelli , S. De Grandi , S. Molendi , G. Zamorani , E. Zucca

The cluster A3627 was recently recognized to be a very massive, nearby cluster in a galaxy survey close to the galactic plane. We are reporting on ROSAT PSPC observations of this object which confirm that the cluster is indeed very massive.…

天体物理学 · 物理学 2009-10-28 Hans Böhringer , Doris M. Neumann , Sabine Schindler , Renee C. Kraan-Korteweg

We present an X-ray analysis of the rich cluster ABCG 85 based on ROSAT PSPC data. By applying an improved wavelet analysis, we show that our view of this cluster is notably changed from what was previously believed (a main region and a…

天体物理学 · 物理学 2008-02-03 V. Pislar , F. Durret , D. Gerbal , G. B. Lima Neto , E. Slezak

We present the results of a pointed ROSAT PSPC observation of the cluster A3558 which is part of the core of the Shapley Concentration. The X-ray brightness distribution can be fitted as the sum of an elliptical King law, with a major core…

天体物理学 · 物理学 2007-05-23 S. Bardelli , E. Zucca , A. Malizia , G. Zamorani , R. Scaramella , G. Vettolani

We have analyzed the ROSAT HRI image and PSPC spectra of Abell~4059. The most striking feature of the X-ray image is the two X-ray holes and an orthogonal X-ray bar in the center of the cluster. It is likely that the radio plasma from the…

天体物理学 · 物理学 2009-10-30 Z. Huang , C. L. Sarazin

We examine Suzaku, XMM-Newton, and Chandra observations of the Abell 2029/2033 system to investigate the nature of a bridge of X-ray emission joining the two galaxy clusters. By modelling the contributions from the outskirts of the two…

宇宙学与河外天体物理 · 物理学 2021-10-27 M. S. Mirakhor , S. A. Walker , J. Runge

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 an analysis of a Chandra observation of the cluster of galaxies Abell 3581. We discover the presence of a point-source in the central dominant galaxy which is coincident with the core of the radio source PKS…

天体物理学 · 物理学 2009-09-17 R. M. Johnstone , A. C. Fabian , R. G. Morris , G. B. Taylor

We present results and an analysis of a ROSAT PSPC pointed observation of the galaxy cluster CL0939+472. This very rich and very distant cluster is known to contain an unusually high fraction of blue and E+A galaxies, and a lot of merging…

天体物理学 · 物理学 2007-05-23 S. Schindler , J. Wambsganss

We present the results of a combined study of ASCA and ROSAT observations of the distant cluster Abell 2390.We determine the surface brightness profile and the gas density distribution of the cluster from the ROSAT PSPC and HRI data. A…

天体物理学 · 物理学 2007-05-23 H. Boehringer , Y. Tanaka , R. F. Mushotzky , Y. Ikebe , M. Hattori

We present an analysis of the hard X-ray emission from the central region of Abell 3667 using deep NuSTAR observations. While previous studies on the nature of the hard X-ray excess have been controversial, our analysis of the central…

高能天体物理现象 · 物理学 2025-07-23 Mohammad S. Mirakhor , Stephen A. Walker

An analysis of a ROSAT/HRI observation of the optically rich, gravitationally lensing galaxy cluster CL0500-24 (or Abell S0506) is presented. We show that the X-ray luminosity of this supposedly rich cluster is relatively low at…

天体物理学 · 物理学 2007-05-23 Sabine Schindler , Joachim Wambsganss

We present a detailed spectral and spatial analysis of the X-ray properties of the compact and unusual radio galaxy 3C 346, combining information from ROSAT and ASCA. The dominant component of X-ray emission (~ 10^44 ergs/s in each of the…

天体物理学 · 物理学 2009-10-31 D. M. Worrall , M. Birkinshaw

We report results of an 18 ks exposure with the ACIS instrument on Chandra of the powerful z = 0.62 radio galaxy 3C 220.1. The X-ray emission separates into cluster gas of emission-weighted kT ~ 5 keV and 0.7-12 keV luminosity (to a radius…

天体物理学 · 物理学 2009-11-06 D. M. Worrall , M. Birkinshaw , M. J. Hardcastle , C. R. Lawrence

We present a new X-ray analysis mainly based on ROSAT HRI data. The HRI spatial resolution combined with an improved wavelet analysis method and with complementary radio and optical data provides new results compared to a previous paper…

天体物理学 · 物理学 2007-05-23 G. B. Lima Neto , V. Pislar , F. Durret , D. Gerbal , E. Slezak

We report Suzaku observations of the galaxy cluster Abell 1795 that extend to r_200 ~ 2 Mpc, the radius within which the mean cluster mass density is 200 times the cosmic critical density. These observations are the first to probe the state…

We present the results of two (101 ks total) Chandra observations of the z=0.778 optically selected lensing cluster RCS022434-0002.5, along with weak lensing and dynamical analyses of this object. An X-ray spectrum extracted within R(2500)…

We present results of ROSAT/PSPC and HRI observations of the AWM7 group of galaxies, which is a poor galaxy cluster and forms part of the Perseus-Pisces filament. The X-ray emission originates from intracluster gas at temperatures of 1.7 to…

天体物理学 · 物理学 2016-08-30 Doris M. Neumann , Hans Boehringer

The X-ray telescope eROSITA onboard the newly launched SRG mission serendipitously observed the galaxy cluster A3408 ($z=0.0420$) during the PV observation of the AGN 1H0707-495. Despite its brightness and large extent, it has not been…

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