activity
20022018
most citedRadiation hydrodynamics integrated in the code PLUTO

55 citations · 368 across the 22 of their papers we have counts for

collaborators

23 papers

astro-ph.SR2018★ 27 cited

The bipolar jet of the symbiotic star R Aquarii: A study of its morphology using the high-resolution HST WFC3/UVIS camera

Stanislav Melnikov, Matthias Stute, Jochen Eisloeffel

R Aqr is a symbiotic binary system consisting of a Mira variable with a pulsation period of 387 days and a hot companion which is presumably a white dwarf with an accretion disk. T…

astro-ph.SR2017★ 54 cited

SPHERE / ZIMPOL observations of the symbiotic system R Aqr. I. Imaging of the stellar binary and the innermost jet clouds

H. M. Schmid, A. Bazzon, J. Milli +40

R Aqr is a symbiotic binary system consisting of a mira variable, a hot companion with a spectacular jet outflow, and an extended emission line nebula. We have used R Aqr as test t…

astro-ph.SR2015★ 30 cited

A Pilot Deep Survey for X-Ray Emission from fuvAGB Stars

R. Sahai, J. Sanz-Forcada, C. Sanchez Contreras +1

We report the results of a pilot survey for X-ray emission from a newly discovered class of AGB stars with far-ultraviolet excesses (fuvAGB stars) using XMM-Newton and Chandra. We…

astro-ph.SR2014★ 11 cited

3D simulations of disc-winds extending radially self-similar MHD models

Matthias Stute, Jose Gracia, Nektarios Vlahakis +3

Disc-winds originating from the inner parts of accretion discs are considered as the basic component of magnetically collimated outflows. The only available analytical MHD solution…

astro-ph.SR2013★ 18 cited

Young stellar object jet models: From theory to synthetic observations

O. Tesileanu, T. Matsakos, S. Massaglia +9

Astronomical observations, analytical solutions and numerical simulations have provided the building blocks to formulate the current theory of young stellar object jets. Although e…

astro-ph.EP2013★ 55 cited

Radiation hydrodynamics integrated in the code PLUTO

Stefan M. Kolb, Matthias Stute, Wilhelm Kley +1

The transport of energy through radiation is very important in many astrophysical phenomena. In dynamical problems the time-dependent equations of radiation hydrodynamics have to b…