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Suzaku observation of the Galactic supernova remnant CTB 37A (G348.5+0.1)
In this paper, we present the results of the observations of CTB 37A obtained with the X-ray imaging spectrometer onboard the Suzaku satellite. The X-ray spectrum of CTB 37A is fitted well by twoExpand
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Origin of gamma-ray emission in the shell of Cassiopeia A
Context. Non-thermal X-ray emission from the shell of Cassiopeia A (Cas A) has been an interesting subject of study, as it provides information about relativistic electrons and their accelerationExpand
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A Randomised Comparison of the Effects of Nebivolol and Atenolol with and without Chlorthalidone on the Sexual Function of Hypertensive Men
AbstractBackground and objective: Erectile dysfunction, which is common in men with hypertension, has been reported as a common adverse effect of many antihypertensive drug classes, includingExpand
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Uniform Contribution of Supernova Explosions to the Chemical Enrichment of Abell 3112 out to R 200
The spatial distribution of the metals residing in the intra-cluster medium (ICM) of galaxy clusters records all the information on a cluster's nucleosynthesis and chemical enrichment history. WeExpand
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Suzaku Observations of Ejecta-Dominated Galactic Supernova Remnant G346.6-0.2
We present here the results of an X-ray analysis of Galactic supernova remnant G346.6−0.2 observed with Suzaku. K-shell emission lines of Mg, Si, S, Ca and Fe are detected clearly for the first time.Expand
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Overdensity of X-Ray Sources in the Field of Two Nearby Clusters of Galaxies: XMM-Newton View of A 194 and A 1060
Two nearby clusters of galaxies, A194 (z =0 .018) and A1060 (z =0 .0114), have been analyzed for their X-ray point-source properties with XMM-Newton EPIC-PN data. A multi-band source detectionExpand
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Searching for Overionized Plasma in the Gamma-ray-emitting Supernova Remnant G349.7+0.2
G349.7+0.2 is a supernova remnant (SNR) expanding in a dense medium of molecular clouds and interacting with clumps of molecular material emitting gamma-rays. We analyzed the gamma-ray data of theExpand
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Exosat observations of Cygnus X-2 continuum and line spectrum
An analysis of five Exosat observations of Cyg X-2, taken around a full binary orbit is presented. The data were obtained using all instrumentation (1000 lines/mm Transmission Grating Spectrometer,Expand
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Recombining Plasma in the Gamma-ray Emitting Mixed-Morphology Supernova Remnant 3C 391
A group of middle-aged mixed-morphology (MM) supernova remnants (SNRs) interacting with molecular clouds (MC) has been discovered as strong GeV gamma-ray emitters by Large Area Telescope on boardExpand
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PROBING THE COSMIC FILAMENTS BY MEANS OF X-RAY OBSERVATIONS
Recent observations and numerical simulations show that galaxies are not distributed in the Universe randomly. They are placed like the pearls of a necklace. The matter is spread into the space inExpand