52 citations · 511 across the 21 of their papers we have counts for
6 papers · 1 filter
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…
Asymmetric supernova remnants generated by Galactic, massive runaway stars
D. M. -A. Meyer, N. Langer, J. Mackey +2
After the death of a runaway massive star, its supernova shock wave interacts with the bow shocks produced by its defunct progenitor, and may lose energy, momentum, and its spheric…
3D MHD simulation of polarized emission in SN 1006
E. M. Schneiter, P. F. Velázquez, E. M. Reynoso +2
We use three dimensional magnetohydrodynamic (MHD) simulations to model the supernova remnant SN 1006. From our numerical results, we have carried out a polarization study, obtaini…
The XMM-Newton X-ray emission of the SNR N120 in the LMC
Jorge Reyes-Iturbide, Margarita Rosado, Pablo F. Velazquez
We present new XMM-Newton observations of the supernova remnant N120 in the LMC, and numerical simulations on the evolution of this supernova remnant which we compare with the X-ra…
3D numerical model of the Omega Nebula (M17): simulated thermal X-ray emission
J. Reyes-Iturbide, P. F. Velazquez, M. Rosado +3
We present 3D hydrodynamical simulations of the superbubble M17, also known as the Omega nebula, carried out with the adaptive grid code yguazu'-a, which includes radiative cooling…