activity
20032007
most citedMHD simulations of jet acceleration from Keplerian accretion disks: the effects of disk resistivity

203 citations · 203 across the 1 of their papers we have counts for

collaborators

5 papers

astro-ph2007203 cited

MHD simulations of jet acceleration from Keplerian accretion disks: the effects of disk resistivity

C. Zanni, A. Ferrari, R. Rosner +2

Accretion disks and astrophysical jets are used to model many active astrophysical objects, viz., young stars, relativistic stars, and active galactic nuclei. In this paper we pres…

astro-ph2005

Crushing of interstellar gas clouds in supernova remnants. I. The role of thermal conduction and radiative losses

S. Orlando, G. Peres, F. Reale +4

We model the hydrodynamic interaction of a shock wave of an evolved supernova remnant with a small interstellar gas cloud like the ones observed in the Cygnus loop and in the Vela…

astro-ph2003

Morphology of Rising Hydrodynamic and Magneto-hydrodynamic Bubbles from Numerical Simulations

K. Robinson, L. J. Dursi, P. M. Ricker +11

Recent Chandra and XMM-Newton observations of galaxy cluster cooling flows have revealed X-ray emission voids of up to 30 kpc in size that have been identified with buoyant, magnet…

astro-ph2003

On Heavy Element Enrichment in Classical Novae

A. Alexakis, A. C. Calder, A. Heger +10

Many classical nova ejecta are enriched in CNO and Ne. Rosner et al. recently suggested that the enrichment might originate in the resonant interaction between large-scale shear fl…

astro-ph2003

The Response of Model and Astrophysical Thermonuclear Flames to Curvature and Stretch

L. J. Dursi, M. Zingale, A. C. Calder +11

Critically understanding the `standard candle'-like behavior of Type Ia supernovae requires understanding their explosion mechanism. One family of models for Type Ia Supernovae beg…