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On the hydrodynamic interplay between a young nuclear starburst and a central supermassive black hole
(The Astrophysical Journal, 2010)
Super stellar clusters with a bimodal hydrodynamic solution: an approximate analytic approach
(Astronomy and Astrophysics, 2007)
Super stellar clusters with a bimodal hydrodynamic solution: an approximate analytic approach
(Astronomy and Astrophysics, 2007)
Three-dimensional hydrodynamical simulations of the large scale structure of W50-SS433
(Oxford University Press, 2008-12)
We present 3D hydrodynamical simulations of a precessing jet propagating inside a supernova remnant (SNR) shell, particularly applied to the W50-SS433 system in a search for the origin of its peculiar elongated morphology. ...
Acacia caven gum studies of hydrodynamic parameters
(ChemBio Publishers, 2019-02)
The acacia caven gum (ACG) is an exudate from Acacia caven tree, this gum is dissolved in water and purified by precipitation with ethanol. In this paper the intrinsic viscosity, [η], is calculated by dissimilar equations, ...
Young Stellar Clusters with a Schuster Mass Distribution - I: Stationary Winds
(The Astrophysical Journal, 2013)
SPH simulations of clumps formation by dissipative collision of molecular clouds - I. Non magnetic case
(Edp Sciences S A, 2000-02-01)
Computer experiments of interstellar cloud collisions were performed with a new smoothed-particle-hydrodynamics (SPH) code. The SPH quantities were calculated by using spatially adaptive smoothing lengths and the SPH fluid ...
SPH simulations of clumps formation by dissipative collision of molecular clouds - I. Non magnetic case
(Edp Sciences S A, 2000-02-01)
Computer experiments of interstellar cloud collisions were performed with a new smoothed-particle-hydrodynamics (SPH) code. The SPH quantities were calculated by using spatially adaptive smoothing lengths and the SPH fluid ...
Two-dimensional hydrodynamic models of super star clusters with a positive star formation feedback
(The astrophysical journal, 2008)