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相关论文: Long RXTE Observations of A2163

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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

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 report on the RXTE/PCA observation of the X-ray burster 1E1724-3045 located in the globular cluster Terzan 2. The persistent X-ray emission shows a high level of noise variability, the so-called High Frequency Noise (HFN) with a…

天体物理学 · 物理学 2009-09-25 J. F. Olive , D. Barret , L. Boirin , J. E. Grindlay , J. H. Swank , A. P. Smale

In this Letter we present results from INTEGRAL and RXTE observations of the spectral and timing behavior of the High Mass X-ray Binary A 0535+26 during its August/September 2005 normal (type I) outburst with an average flux…

We report the results from a 200 ks Chandra observation of the z=1.786 radio galaxy 3C294 and its cluster environment, increasing by tenfold our earlier observation. The diffuse emission, extending about 100 kpc around the nucleus, has a…

天体物理学 · 物理学 2009-09-17 A. C. Fabian , J. S. Sanders , C. S. Crawford , S. Ettori

Galaxy clusters with signs for a recent merger show in many cases extended diffuse radio features. This emission originates from relativistic electrons which suffer synchrotron losses due to the intra-cluster magnetic field. The mechanisms…

星系天体物理 · 物理学 2015-02-11 A. Drabent , M. Hoeft , R. F. Pizzo , A. Bonafede , R. J. van Weeren , U. Klein

Measurements of the velocities of galaxies thought to be associated with the giant radio galaxy NGC 6251 confirm the presence of a poor cluster with a systemic redshift of z= 0.0244 +/- 0.0004 and a line-of-sight velocity dispersion of…

天体物理学 · 物理学 2016-08-30 P. N. Werner , D. M. Worrall , M. Birkinshaw

We present results from two observations (combined exposure of ~17 ks) of galaxy cluster A2218 using the Advanced CCD Imaging Spectrometer on board the Chandra X-ray Observatory that were taken on October 19, 1999. Using a Raymond-Smith…

天体物理学 · 物理学 2009-11-07 M. E. Machacek , M. W. Bautz , C. R. Canizares , G. P. Garmire

We present results of the first RXTE investigation of hard X-ray emission from normal elliptical galaxies. Joint spectral analysis of RXTE PCA and ASCA GIS data for NGC 4472 and NGC 4649 reveals the presence of about 5 10^-12 erg cm^-2 s^-1…

天体物理学 · 物理学 2009-10-31 Michael Loewenstein , Azita Valinia , Richard Mushotzky

We present high resolution 240 and 607 MHz GMRT radio observations, complemented with 74 MHz archival VLA radio observations of the Ophiuchus cluster of galaxies, whose radio mini-halo has been recently detected at 1400 MHz. We also present…

We present a systematic analysis of the extended X-ray emission discovered around 35 FR II radio galaxies from the revised Third Cambridge catalog (3CR) Chandra Snapshot Survey with redshifts between 0.05 to 0.9. We aimed to (i) test for…

We report about the detection of 10 clusters of galaxies in the ongoing Swift/BAT all-sky survey. This sample, which comprises mostly merging clusters, was serendipitously detected in the 15--55 keV band. We use the BAT sample to…

天体物理学 · 物理学 2008-12-18 M. Ajello , P. Rebusco , N. Cappelluti , O. Reimer , H. Boehringer , J. Greiner , N. Gehrels , J. Tueller , A. Moretti

The binary system, LSI+61 303, is unusual both because of the dramatic, periodic, radio outbursts, and because of its possible association with the 100 MeV gamma-ray source, 2CG135+01. We have performed simultaneous radio and Rossi X-ray…

天体物理学 · 物理学 2009-10-31 F. A. Harrison , P. S. Ray , D. A. Leahy , E. B. Waltman , G. G. Pooley

We present results from the XMM-Newton observation of the non-cooling flow cluster A1060. Large effective area of XMM-Newton enables us to investigate the nature of this cluster in unprecedented detail. From the observed surface brightness…

天体物理学 · 物理学 2015-06-24 Akira Hayakawa , Akio Hoshino , Manabu Ishida , Tae Furusho , Noriko Y. Yamasaki , Takaya Ohashi

Aims: Hete J1900.1-2455 is the seventh known X-ray transient accreting millisecond pulsar and has been in outburst for more than one year. We compared the data on Hete J1900.1-2455 with other similar objects and made an attempt at deriving…

天体物理学 · 物理学 2009-11-11 M. Falanga , J. Poutanen , E. W. Bonning , L. Kuiper , J. M. Bonnet-Bidaud , A. Goldwurm , W. Hermsen , L. Stella

The GOES X1.5 class flare that occurred on August 30,2002 at 1327:30 UT is one of the few events detected so far at submillimeter wavelengths. We present a detailed analysis of this flare combining radio observations from 1.5 to 212 GHz (an…

太阳与恒星天体物理 · 物理学 2015-05-13 C. G. Gimenez de Castro , G. Trottet , A. Silva-Valio , S. Krucker , J. E. R. Costa , P. Kaufmann , E. Correia , H. Levato

We performed GMRT low frequency observations of the radio halos, relics and new candidates belonging to the GMRT Radio Halo Cluster Sample first observed at 610 MHz. High sensitivity imaging was performed using the GMRT at 325 MHz and 240…

We present the results of a ~230 ks long X-ray observation of the relativistic double-pulsar system PSR J0737-3039 obtained with the XMM-Newton satellite in 2006 October. We confirm the detection in X-rays of pulsed emission from PSR…

天体物理学 · 物理学 2009-02-23 A. Pellizzoni , A. Tiengo , A. De Luca , P. Esposito , S. Mereghetti

The nonthermal particle content of galaxy clusters should in part have a cosmological component generated during the early starburst phase of the member galaxies. This is reviewed in the framework of a simple cluster formation model…

天体物理学 · 物理学 2009-10-31 H. J. Voelk , A. M. Atoyan

We report on the discovery of 10 additional galaxy clusters detected in the ongoing Swift/BAT all-sky survey. Among the newly BAT-discovered clusters there are: Bullet, Abell 85, Norma, and PKS 0745-19. Norma is the only cluster, among…

宇宙学与河外天体物理 · 物理学 2015-05-20 M. Ajello , P. Rebusco , N. Cappelluti , O. Reimer , H. Boehringer , V. La Parola , G. Cusumano