40 citations · 55 across the 7 of their papers we have counts for
7 papers
An analysis of the turbulence in the central region of the Orion Nebula (M42) -- II. homogeneity and power-spectrum analyses
G. A. Anorve-Zeferino
In this second communication we continue our analysis of the turbulence in the Huygens Region of the Orion Nebula (M 42). We calculate the associated transverse structure functions…
An analysis of the turbulence in the central region of M 42 through structure functions
G. A. Anorve-Zeferino
Here, we analyse the character of the turbulence of the Huygens Region in the Orion Nebula (M 42) using structure functions. We compute the second order structure function of a hig…
Gravitational and mass distribution effects on stationary superwinds
Gabriel Alejandro Añorve-Zeferino
Here, we model the effect of non-uniform dynamical mass distributions and their associated gravitational fields on the stationary galactic superwind solution. We do this by conside…
Gravitational and mass distribution effects on stationary superwinds II. Extended dark matter haloes
G. A. Añorve-Zeferino, M. G. Corona-Galindo
In this second part, we generalize the results of the previous paper. We present an analytic superwind solution considering extended gravitationally-interacting dark-matter and bar…
Gravitational and mass distribution effects on stationary superwinds I
G. A. Añorve-Zeferino, M. G. Corona-Galindo
Here, we model the effect of non-uniform dynamical mass distributions and their associated gravitational fields on the stationary galactic superwind solution. We do this by conside…
On the X-ray emission from massive star clusters and their evolving superbubbles II. Detailed analytics and observational effects
G. A. Añorve-Zeferino, G. Tenorio-Tagle, S. Silich
In this work, we present a comprehensive X-ray picture of the interaction between a super star cluster and the ISM. In order to do that, we compare and combine the X-ray emission f…
On the X-ray Emission from Massive Star Clusters and their Evolving Superbubbles
Sergiy Silich, Guillermo Tenorio-Tagle, Gabriel Alejandro Anorve Zeferino
The X-ray emission properties from the hot thermalized plasma that results from the collisions of individual stellar winds and supernovae ejecta within rich and compact star cluste…