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

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16 papers · 1 filter

astro-ph2007★ 49 cited

Two-component jet simulations: I. Topological stability of analytical MHD outflow solutions

T. Matsakos, K. Tsinganos, N. Vlahakis +3

Observations of collimated outflows in young stellar objects indicate that several features of the jets can be understood by adopting the picture of a two-component outflow, wherei…

astro-ph2005★ 32 cited

Nonradial and nonpolytropic astrophysical outflows VIII. A GRMHD generalization for relativistic jets

Z. Meliani, C. Sauty, N. Vlahakis +2

Steady axisymmetric outflows originating at the hot coronal magnetosphere of a Schwarzschild black hole and surrounding accretion disk are studied in the framework of general relat…

astro-ph2004★ 32 cited

Nonradial and nonpolytropic astrophysical outflows VI. Overpressured winds and jets

Christophe Sauty, Edoardo Trussoni, Kanaris Tsinganos

By means of a nonlinear separation of the variables in the governing full set of the magnetohydrodynamic (MHD) equations for axisymmetric plasmas we analyse an exact model for magn…

astro-ph2003★ 26 cited

A multi-wavelength test of the FR~I - BL Lac unifying model

E. Trussoni, A. Capetti, A. Celotti +2

We collect multi-wavelength measurements of the nuclear emission of 20 low luminosity FR I radio-galaxies to test the viability of the FR I - BL Lac unifying model. Although poorly…

astro-ph2002★ 55 cited

Nonradial and nonpolytropic astrophysical outflows. V. Acceleration and collimation of self-similar winds

C. Sauty, E. Trussoni, K. Tsinganos

An exact model for magnetized and rotating outflows, underpressured at their axis, is analysed by means of a nonlinear separation of the variables in the two-dimensional governing…

astro-ph2002★ 45 cited

The X-ray emission from Nova V382 Velorum: II. The super-soft component observed with BeppoSAX

M. Orio, A. N. Parmar, J. Greiner +3

Nova Velorum 1999 (V382 Vel) was observed by BeppoSAX 6 months after optical maximum and was detected as a bright X-ray supersoft source, with a count rate 3.454+-0.002 cts/s in th…