activity
20172022
most citedPSR J2030+4415's Remarkable Bow Shock, PWN and Filament

22 citations · 90 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2022★ 10 cited

Chandra measurements of gas homogeneity and turbulence at intermediate radii in the Perseus Cluster

Martijn de Vries, Adam B. Mantz, Steven W. Allen +6

We present a Chandra study of surface brightness fluctuations in the diffuse intracluster medium of the Perseus Cluster. Our study utilizes deep, archival imaging of the cluster co…

astro-ph.HE2022

Late-Time X-ray Observations of the Transient Source Cygnus A-2

Bradford Snios, Martijn De Vries, Paul E. J. Nulsen +3

We examine Chandra observations of the powerful Fanaroff-Riley class II (FR II) radio galaxy Cygnus A for an X-ray counterpart to the radio transient Cygnus A-2 that was first dete…

astro-ph.HE2020★ 22 cited

PSR J2030+4415's Remarkable Bow Shock, PWN and Filament

Martijn de Vries, Roger W. Romani

We report on new X-ray and optical observations of PSR J2030+4415, a Gamma-ray Pulsar with an H bow shock. These data reveal the velocity structure of the bow shock apex and res…

astro-ph.HE2018★ 9 cited

Simulations of the merging cluster of galaxies Cygnus A

Timo Halbesma, Julius Donnert, Martijn de Vries +1

The archetype FR-II galaxy Cygnus A lies in a moderately rich cluster about to undergo a major merger. We study the pre-merger Cygnus cluster environment using smoothed particle hy…

astro-ph.GA2018★ 12 cited

Signatures of multiple episodes of AGN activity in the core of Abell 1795

Georgi Kokotanekov, Michael W. Wise, Martijn de Vries +1

In this paper we analyze AGN activity signatures in the rich nearby galaxy cluster Abell 1795 aiming to confirm and characterize the long-term feedback history in the system. We co…

astro-ph.HE2018★ 18 cited

Detection of non-thermal X-ray emission in the lobes and jets of Cygnus A

M. N. de Vries, M. W. Wise, D. Huppenkothen +7

We present a spectral analysis of the lobes and X-ray jets of Cygnus A, using more than 2 Ms of observations. The X-ray jets are misaligned with the radio jets a…