output
20022009
most citedShocks and cold fronts in galaxy clusters

755 citations

Showing 2009Show all

6 papers · 1 filter

nlin.CD20097 cited

Using Resonances to Control Chaotic Mixing within a Translating and Rotating Droplet

Rodolphe Chabreyrie, Dmitri Vainchtein, Cristel Chandre +2

Enhancing and controlling chaotic advection or chaotic mixing within liquid droplets is crucial for a variety of applications including digital microfluidic devices which use micro…

astro-ph.HE200946 cited

Luminosity functions of LMXBs in Centaurus A: globular clusters versus the field

R. Voss, M. Gilfanov, G. R. Sivakoff +16

We study the X-ray luminosity function (XLF) of low mass X-ray binaries (LMXB) in the nearby early-type galaxy Centaurus A, concentrating primarily on two aspects of binary populat…

astro-ph.HE200994 cited

Advection/Diffusion of Large-Scale B-Field in Accretion Disks

R. V. E. Lovelace, D. M. Rothstein, G. S. Bisnovatyi-Kogan

Activity of the nuclei of galaxies and stellar mass systems involving disk accretion to black holes is thought to be due to (1) a small-scale turbulent magnetic field in the disk (…

cond-mat.other200943 cited

Dynamics of a many-particle Landau-Zener model: inverse sweep

A. P. Itin, P. Törmä

We consider dynamics of a slowly time-dependent Dicke model, which represents a many-body generalization of the Landau-Zener model. In particular, the model describes narrow Feshba…

astro-ph.EP200964 cited

On the protection of extrasolar Earth-like planets around K/M stars against galactic cosmic rays

J. -M. Grießmeier, A. Stadelmann, J. L. Grenfell +2

Previous studies have shown that extrasolar Earth-like planets in close-in habitable zones around M-stars are weakly protected against galactic cosmic rays (GCRs), leading to a str…

astro-ph.EP200955 cited

Intermittent turbulence, noisy fluctuations and wavy structures in the Venusian magnetosheath and wake

Z. Vörös, T. L. Zhang, M. P. Leubner +3

Recent research has shown that distinct physical regions in the Venusian induced magnetosphere are recognizable from the variations of strength of the magnetic field and its wave/f…