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20022009
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

collaborators

11 papers

astro-ph.SR200921 cited

Detection of X-rays from the jet-driving Symbiotic Star MWC 560

Matthias Stute, Raghvendra Sahai

We report the detection of X-ray emission from the jet-driving symbiotic star MWC 560. We observed MWC 560 with XMM-Newton for 36 ks. We fitted the spectra from the EPIC pn, MOS1 a…

astro-ph.SR200916 cited

Mid-IR period-magnitude relations for AGB stars

I. S. Glass, M. Schultheis, J. A. D. L. Blommaert +3

Asymptotic Giant Branch variables are found to obey period-luminosity relations in the mid-IR similar to those seen at K_S (2.14 microns), even at 24 microns where emission from ci…

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…