activity
19952010
most citedDraping of Cluster Magnetic Fields over Bullets and Bubbles -- Morphology and Dynamic Effects

249 citations · 1.1k across the 19 of their papers we have counts for

collaborators

19 papers

astro-ph.CO2010★ 90 cited

Recombinations to the Rydberg States of Hydrogen and Their Effect During the Cosmological Recombination Epoch

J. Chluba, G. M. Vasil, L. J. Dursi

In this paper we discuss the effect of recombinations to highly excited states (n > 100) in hydrogen during the cosmological recombination epoch. For this purpose, we developed a n…

astro-ph.CO2009★ 93 cited

Detecting the orientation of magnetic fields in galaxy clusters

Christoph Pfrommer, L. Jonathan Dursi

Clusters of galaxies, filled with hot magnetized plasma, are the largest bound objects in existence and an important touchstone in understanding the formation of structures in our…

astro-ph2007★ 249 cited

Draping of Cluster Magnetic Fields over Bullets and Bubbles -- Morphology and Dynamic Effects

L. J. Dursi, C. Pfrommer

High-resolution X-ray observations have revealed cavities and `cold fronts' with sharp edges in temperature, density, and metallicity within galaxy clusters. Their presence poses a…

astro-ph2007★ 43 cited

Bubble-Wrap for Bullets: The Stability Imparted By A Thin Magnetic Layer

L. J. Dursi

There has been significant recent work which examines a situation where a thin magnetic layer is `draped' over a core merging into a larger cluster; the same process also appears t…

astro-ph2006★ 46 cited

Propagation of the First Flames in Type Ia Supernovae

M. Zingale, L. J. Dursi

We consider the competition of the different physical processes that can affect the evolution of a flame bubble in a Type Ia supernovae -- burning, turbulence and buoyancy. Even in…

astro-ph2005★ 31 cited

Local Ignition in Carbon/Oxygen White Dwarfs -- I: One-zone Ignition and Spherical Shock Ignition of Detonations

L. Jonathan Dursi, F. X. Timmes

The details of ignition of Type Ia supernovae remain fuzzy, despite the importance of this input for any large-scale model of the final explosion. Here, we begin a process of under…