activity
19962025
most citedEvolution of Buoyant Bubbles in M87

719 citations · 10.2k across the 157 of their papers we have counts for

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Showing 2016Show all

10 papers · 1 filter

astro-ph.HE2016★ 57 cited

Deep Chandra observations of NGC 1404: cluster plasma physics revealed by an infalling early-type galaxy

Yuanyuan Su, Ralph P. Kraft, Elke Roediger +6

The intracluster medium (ICM), as a magnetized and highly ionized fluid, provides an ideal laboratory to study plasma physics under extreme conditions that cannot yet be achieved o…

astro-ph.HE2016★ 23 cited

Capturing the 3D Motion of an Infalling Galaxy via Fluid Dynamics

Yuanyuan Su, Ralph P. Kraft, Paul E. J. Nulsen +6

The Fornax Cluster is the nearest galaxy cluster in the southern sky. NGC 1404 is a bright elliptical galaxy falling through the intracluster medium of the Fornax Cluster. The shar…

astro-ph.HE2016★ 40 cited

Polarization and long-term variability of Sgr A* X-ray echo

E. Churazov, I. Khabibullin, G. Ponti +1

We use a model of the molecular gas distribution within ~100 pc from the center of the Milky Way (Kruijssen, Dale & Longmore) to simulate time evolution and polarization properties…

astro-ph.HE2016★ 47 cited

Not that long time ago in the nearest galaxy: 3D slice of molecular gas revealed by a 110 years old flare of Sgr A*

E. Churazov, I. Khabibullin, R. Sunyaev +1

A powerful outburst of X-ray radiation from the supermassive black hole Sgr A* at the center of the Milky Way is believed to be responsible for the illumination of molecular clouds…

astro-ph.CO2016★ 32 cited

Arithmetic with X-ray images of galaxy clusters: effective equation of state for small-scale perturbations in the ICM

E. Churazov, P. Arevalo, W. Forman +4

We discuss a novel technique of manipulating X-ray images of galaxy clusters to reveal the nature of small-scale density/temperature perturbations in the intra cluster medium (ICM)…

astro-ph.HE2016★ 7 cited

Polarization of thermal bremsstrahlung emission due to electron pressure anisotropy

S. Komarov, I. Khabibullin, E. Churazov +1

Astrophysical plasmas are typically magnetized, with the Larmor radii of the charged particles many orders of magnitude smaller than their collisional mean free paths. The fundamen…