activity
20202023
most citedHidden Cooling Flows in Clusters of Galaxies

37 citations · 255 across the 16 of their papers we have counts for

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Showing astro-ph.HEShow all

5 papers · 1 filter

astro-ph.HE2023★ 16 cited

Measuring the hot ICM velocity structure function using XMM-Newton observations

Efrain Gatuzz, R. Mohapatra, C. Federrath +4

It has been shown that the gas velocities within the intracluster medium (ICM) can be measured by applying novel XMM-Newton EPIC-pn energy scale calibration, which uses instrumenta…

astro-ph.HE2023★ 12 cited

Chemical enrichment of the ICM within the Virgo cluster I: radial profiles

Efrain Gatuzz, J. Sanders, K. Dennerl +8

We present a detailed analysis of the elemental abundances distribution of the Virgo cluster using {\it XMM-Newton} observations. We included in the analysis a new EPIC-pn energy s…

astro-ph.HE2022★ 3 cited

Possible non-thermal origin of the hard X-ray emission in the merging galaxy cluster SPT-CL J2031-4037

M. S. Mirakhor, S. A. Walker, J. Runge +1

Non-thermal emission from clusters of galaxies at the high-energy X-ray regime has been searched with various instruments, but the detection significance of this emission has yet b…

astro-ph.HE2021★ 30 cited

Far UV and Optical Emissions from Three Very Large Supernova Remnants Located at Unusually High Galactic Latitudes

Robert A. Fesen, Marcel Drechsler, Kathryn E. Weil +9

Galactic supernova remnants (SNRs) with angular dimensions greater than a few degrees are relatively rare, as are remnants located more than ten degrees off the Galactic plane. Her…

astro-ph.HE2020★ 24 cited

G107.0+9.0: A New Large Optically Bright, Radio and X-Ray Faint Galactic Supernova Remnant in Cepheus

Robert A. Fesen, Kathryn E. Weil, John C. Raymond +7

Wide-field H-alpha images of the Galactic plane have revealed a new supernova remnant (SNR) nearly three degrees in diameter centred at l = 107.0, b = +9.0. Deep and higher resolut…