26 citations · 130 across the 9 of their papers we have counts for
9 papers
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…
The sculpting of rectangular and jet-like morphologies in supernova remnants by anisotropic equatorially-confined progenitor stellar winds
P. F. Velazquez, D. M. -A. Meyer, A. Chiotellis +5
Thermonuclear and core-collapse supernova remnants (SNRs) are the nebular leftovers of defunct stars. Their morphology and emission properties provide insights into the evolutionar…
Rectangular core-collapse supernova remnants: application to Puppis A
D. M. -A. Meyer, P. F. Velazquez, O. Petruk +9
Core-collapse supernova remnants are the gaseous nebulae of galactic interstellar media (ISM) formed after the explosive death of massive stars. Their morphology and emission prope…
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…
The soft and hard X-rays thermal emission from star cluster winds with a supernova explosion
A. Castellanos-Ramirez, A. Rodriguez-Gonzalez, A. Esquivel +3
Massive young star clusters contain dozens or hundreds of massive stars that inject mechanical energy in the form of winds and supernova explosions, producing an outflow which expa…
Measuring social complexity and the emergence of cooperation from entropic principles
O. López-Corona, P. Padilla, A. Huerta +5
Assessing quantitatively the state and dynamics of a social system is a very difficult problem. It is of great importance for both practical and theoretical reasons such as establi…
An asymmetric jet launching model for the protoplanetary nebula CRL 618
P. F. Velazquez, A. Riera, A. C. Raga +1
We propose an asymmetrical jet ejection mechanism in order to model the mirror symmetry observed in the lobe distribution of some protoplanetary nebulae (pPNe), such as the pPN CRL…
A Stellar Wind Origin for the G2 Cloud: Three-Dimensional Numerical Simulations
Fabio De Colle, A. C. Raga, Flavio F. Contreras-Torres +1
We present 3D, adaptive mesh refinement simulations of G2, a cloud of gas moving in a highly eccentric orbit towards the galactic center. We assume that G2 originates from a stella…
X-ray emission and dynamics from large diameter superbubbles: The case of N 70 superbubble
Ary Rodríguez-González, Pablo F. Velázquez, Margarita Rosado +3
The morphology, dynamics and thermal X-ray emission of the superbubble N70 is studied by means of 3D hydrodynamical simulations, carried out with the {\sc{yguazú-a}} code. We have…