activity
19942013
most citedA disk-wind model with correct crossing of all MHD critical surfaces

119 citations · 528 across the 22 of their papers we have counts for

collaborators

22 papers

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.SR2012★ 12 cited

Velocity asymmetries in YSO jets: Intrinsic and extrinsic mechanisms

T. Matsakos, N. Vlahakis, K. Tsinganos +7

It is a well established fact that some YSO jets (e.g. RW Aur) display different propagation speeds between their blue and red shifted parts, a feature possibly associated with the…

astro-ph.IM2010

A decline and fall in the future of Italian Astronomy?

Angelo Antonelli, Vincenzo Antonuccio-Delogu, Andrea Baruffolo +89

On May 27th 2010, the Italian astronomical community learned with concern that the National Institute for Astrophysics (INAF) was going to be suppressed, and that its employees wer…

astro-ph.CO2010★ 19 cited

Relativistic spine jets from Schwarzschild black holes: "Application to AGN radioloud sources"

Z. Meliani, C. Sauty, K. Tsinganos +2

The two types of Fanaroff-Riley radio loud galaxies, FRI and FRII, exhibit strong jets but with different properties. These differences may be associated to the central engine and/…

astro-ph.GA2009

Two-component jet simulations: Combining analytical and numerical approaches

T. Matsakos, S. Massaglia, E. Trussoni +4

Recent observations as well as theoretical studies of YSO jets suggest the presence of two steady components: a disk wind type outflow needed to explain the observed high mass loss…

astro-ph.GA2009★ 31 cited

Two-component jet simulations: II. Combining analytical disk and stellar MHD outflow solutions

T. Matsakos, S. Massaglia, E. Trussoni +4

Theoretical arguments along with observational data of YSO jets suggest the presence of two steady components: a disk wind type outflow needed to explain the observed high mass los…