15 citations · 22 across the 6 of their papers we have counts for
6 papers
Unveiling the collision between molecular outflows: observational evidence and hydrodynamic simulations
E. Cohen Arazi, P. F. Velázquez, M. E. Ortega +5
We present an unexplored scenario for interpreting the outflows in the EGO G338.92+0.55 (b) region (hereafter, EGO G338). Within this framework, we investigate the hypothesis that…
Effects of Radiative Transfer on the Observed Anisotropy in MHD Turbulent Molecular Simulations
D. Hernández-Padilla, A. Esquivel, A. Lazarian +2
We study the anisotropy of centroid and integrated intensity maps with synthetic observations. We perform post-process radiative transfer including the optically thick regime that…
Simulated non-thermal emission from SNR G1.9+0.3
Marco A. Villagran, D. O. Gómez, P. F. Velázquez +7
Supernova remnants are the nebular leftover of defunct stellar environments, resulting from the interaction between a supernova blastwave and the circumstellar medium shaped by the…
Numerical simulations of the 1840s great eruption of Carinae: I. Revisiting the explosion scenario
R. F. González, Luis A. Zapata, A. C. Raga +3
In this work, we present new two-dimensional hydrodynamical simulations of the major eruption of Car in the 1840s, which resulted in the formation of a bipolar nebula that is c…
3D MHD simulations of the supernova remnant CTB 109
A. Castellanos-Ramírez, P. F. Velázquez, J. Cantó
We examine the evolution and emission of the supernova remnant (SNR) CTB109 using three-dimensional magnetohydrodynamics simulations. The SNR evolves in a medium divided by a plane…
A 3D MHD simulation of SN 1006: a polarized emission study for the turbulent case
P. F. Velázquez, E. M. Schneiter, E. M. Reynoso +6
Three dimensional magnetohydrodynamical simulations were carried out in order to perform a new polarization study of the radio emission of the supernova remnant SN 1006. These simu…