activity
20052026
most cited{\it Suzaku} observation of Galactic supernova remnant CTB 37A (G348.5+0.1)

17 citations · 61 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2026

Weak cool core, weak turbulence: XRISM, XMM-Newton and Chandra spectroscopy of the core of Abell 1413

Egemen Gormez, Murat Hudaverdi

We present the first XRISM spectroscopy of the core of Abell 1413 (z = 0.143), combining 104.7 ks of Resolve with archival XMM-Newton and Chandra spectra of a matched sky region. A…

astro-ph.CO2021★ 9 cited

The Relative Supernovae Contribution to the Chemical Enrichment History of Abell 1837

M. K. Erdim, C. Ezer, O. Ünver +2

In this paper, we report the relative SNe contributions on the metal budget of the ICM of Abell 1837 galaxy cluster at redshift z 0.069. For this purpose, we analysed the hot I…

astro-ph.CO2019★ 4 cited

Chandra observation of a cold front in Abell 2554

M. Kiyami Erdim, Murat Hudaverdi

We present the evidence for the existence of substructure in the cold front cluster A2554 based on a 20.14 ks Chandra observation. Using centroid shift and X-ray brightness concent…

astro-ph.HE2017★ 13 cited

Dynamical history of a binary cluster: Abell 3653

Turgay Caglar, Murat Hudaverdi

We study the dynamical structure of a bimodal galaxy cluster Abell 3653 at z=0.1089 by using combined optical and X-ray data. Observations include archival data from Anglo-Australi…

astro-ph.HE2017★ 8 cited

XMM-Newton view of X-ray overdensities from nearby galaxy clusters: the environmental dependencies

Turgay Caglar, Murat Hudaverdi

In this work, we studied ten nearby (0.038) galaxy clusters to understand possible interactions between hot plasma and member galaxies. A multi-band source detection was…

astro-ph.HE2011★ 17 cited

{\it Suzaku} observation of Galactic supernova remnant CTB 37A (G348.5+0.1)

A. Sezer, F. Gök, M. Hudaverdi +1

We present here the results of the observation of CTB 37A obtained with the X-ray Imaging Spectrometer onboard the {\it Suzaku} satellite. The X-ray spectrum of CTB 37A is well fit…