activity
20142021
most citedCompressible flow in front of an axisymmetric blunt object: analytic approximation and astrophysical implications

7 citations · 21 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2021★ 4 cited

Protruding bullet heads indicating dark matter pull

Uri Keshet, Itay Raveh, Yossi Naor

A clump moving through the intracluster medium of a galaxy cluster can drive a bow shock trailed by a bullet-like core. In some cases, such as in the prototypical Bullet cluster, X…

astro-ph.HE2020★ 4 cited

Advection by large-scale spiral flows in galaxy clusters

Yossi Naor, Uri Keshet

The intracluster medium of a galaxy cluster often shows an extended quasi-spiral structure, accentuated by tangential discontinuities known as cold fronts (CFs). These discontinuit…

astro-ph.HE2020★ 6 cited

Deprojecting galaxy-cluster cold fronts: evidence for bulk, magnetised spiral flows

Yossi Naor, Uri Keshet, Qian Wang +1

Tangential discontinuities known as cold fronts (CFs) are abundant in groups and clusters of galaxies (GCs). The relaxed, spiral-type CFs were initially thought to be isobaric, but…

astro-ph.EP2016★ 7 cited

Compressible flow in front of an axisymmetric blunt object: analytic approximation and astrophysical implications

Uri Keshet, Yossi Naor

Compressible flows around blunt objects have diverse applications, but current analytic treatments are inaccurate and limited to narrow parameter regimes. We show that the gas-dyna…

astro-ph.GA2015

Magnetohydrodynamics using path or stream functions

Yossi Naor, Uri Keshet

Magnetization in highly conductive plasmas is ubiquitous to astronomical systems. Flows in such media can be described by three path functions , or, for a steady flow, by two…

astro-ph.IM2014

Compressible flow in front of an axisymmetric blunt object

Uri Keshet, Yossi Naor

Compressible flows around blunt objects have diverse applications, but present analytic treatments are inaccurate and limited to narrow parameter regimes. We show that the flow in…