activity
20022018
most citedJet/cloud collision, 3D gasdynamic simulations of HH 110

106 citations · 472 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.HE2018★ 10 cited

New perspectives on the supernova remnant Puppis A based on a radio polarization study

E. M. Reynoso, P. F. Velázquez, S. Cichowolski

We present a polarization study towards the supernova remnant (SNR) Puppis A based on original observations performed with the Australia Telescope Compact Array (ATCA). Based on th…

astro-ph.GA2016★ 3 cited

The time evolution of HH~2 from four epochs of HST images

A. C. Raga, B. Reipurth, P. F. Velázquez +2

We have analyzed four epochs of H and [S~II] HST images of the HH~1/2 outflow (covering a time interval from 1994 to 2014) to determine proper motions and emission line fluxes o…

astro-ph.SR2016★ 20 cited

Observations and 3D Hydrodynamical models of planetary nebulae with Wolf Rayet type central stars

J. S. Rechy-García, P. F. Velázquez, M. Peña +1

We present high-resolution, long-slit spectroscopic observations of two planetary nebulae with [WC] central stars located near the galactic bulge, M 1-32 and M 3-15. The observatio…

astro-ph.HE2014★ 13 cited

Diffuse X-ray emission from the superbubbles N 70 and N 185 in the Large Magellanic Cloud

Jorge Reyes-Iturbide., Margarita Rosado., Ary Rodríguez-González. +3

We present a study of the diffuse X-ray emission from superbubbles N 70 (DEM L301) and N 185 (DEM L25) located in the Large Magellanic Cloud, based on data from the XMM-Newton Sate…

astro-ph.SR2014★ 9 cited

Modelling the 3D morphology and proper motions of the planetary nebula NGC 6302

L. Uscanga, P. F. Velázquez, A. Esquivel +3

We present 3D hydrodynamical simulations of an isotropic fast wind interacting with a previously ejected toroidally-shaped slow wind in order to model both the observed morphology…

astro-ph.HE2011

The cometary cavity created by an aligned streaming environment/collimated outflow interaction

D. López-Cámara, A. Esquivel, J. Cantó +3

We present a "thin shell" model of the interaction of a biconical outflow and a streaming environment (aligned with the direction of the flow), as well as numerical (axisymmetric)…