M. Hudaverdi

Publications40
h-index4
Citations61
Highly Influential Citations12
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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 two… Expand
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Non-Uniform Temperature Distribution in the Galaxy Clusters 2A 0335+096 and Abell 496 Observed by XMM-Newton
We present the XMM-Newton results of the galaxy clusters 2A 0335+096 and A496. From an investigation of 2-dimensional ICM profiles, we obtained new features related to dynamical activities in the… 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 detection… Expand
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ASCA and XMM-Newton observations of A2029
Abstract The X-ray data of A2029 obtained with XMM-Newton show no evidence of an embedded AGN in the central region of this cluster, which was suggested from the analysis of restored ASCA image data,… Expand
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Dynamical history of a binary cluster : Abell 3653
We study the dynamical structure of a bimodal galaxy cluster Abell 3653 at z = 0.1089 using optical and X-ray data. Observations include archival data from the Anglo-Australian Telescope, X-ray… Expand
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The correlations of space weather and satellite anomalies: RASAT
The main focus of this work is to review documented operational anomalies for Turkish Remote Sensing Satellite of RASAT, by assessing the identification and estimation of potential source of space… Expand
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X-ray Observation of an Ongoing Merger at the Galaxy Cluster Abell 3653
Non-Uniformity in Temperature and Abundance
An X-ray study of the well-known galactic shell-type supernova remnants
Characterizing decaying dark matter: X-ray emission from sterile neutrinos
Recently, an unknown emission line at E $\sim$3.5 keV from several astrophysical objects has been detected. The line is suggested to be originating from decaying dark matter particles. The results… Expand