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most citedX-ray emission from Planetary Nebulae. I. Spherically symmetric numerical simulations

30 citations · 93 across the 6 of their papers we have counts for

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astro-ph2008

Hydrodynamical simulations of the jet in the symbiotic star MWC 560. II. Simulations beyond density balance

Matthias Stute

(Abridged) In the first paper of this series, we presented hydrodynamical simulations with radiative cooling of jet models with parameters representative of the symbiotic system MW…

astro-ph200813 cited

Stability and structure of analytical MHD jet formation models with a finite outer disk radius

Matthias Stute, Kanaris Tsinganos, Nektarios Vlahakis +2

(Abridged) Finite radius accretion disks are a strong candidate for launching astrophysical jets from their inner parts and disk-winds are considered as the basic component of such…

astro-ph200713 cited

Hydrodynamical simulations of the jet in the symbiotic star MWC 560 III. Application to X-ray jets in symbiotic stars

Matthias Stute, Raghvendra Sahai

In papers I and II in this series, we presented hydrodynamical simulations of jet models with parameters representative of the symbiotic system MWC 560. These were simulations of a…

astro-ph200630 cited

X-ray emission from Planetary Nebulae. I. Spherically symmetric numerical simulations

Matthias Stute, Raghvendra Sahai

(abridged) The interaction of a fast wind with a spherical Asymptotic Giant Branch (AGB) wind is thought to be the basic mechanism for shaping Pre-Planetary Nebulae (PPN) and later…

astro-ph2005

Effects of a solid surface on jet formation around neutron stars

Matthias Stute, Jose Gracia, Max Camenzind

We present two numerical simulations of an accretion flow from a rotating torus onto a compact object with and without a solid surface -- representing a neutron star and a black ho…

astro-ph2005

Are jets in symbiotic stars driven by magnetic fields?

Matthias Stute, Max Camenzind

We compare two scenarios to launch jets -- formation by MHD processes or formation by thermal pressure in the boundary layer (BL) -- with respect to their compatibility with observ…