52 citations · 511 across the 21 of their papers we have counts for
21 papers
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…
3D MHD astrospheres: applications to IRC-10414 and Betelgeuse
D. M. -A. Meyer, A. Mignone, M. Petrov +3
A significative fraction of all massive stars in the Milky Way move supersonically through their local interstellar medium (ISM), producing bow shock nebulae by wind-ISM interactio…
Proper motions of the HH1 jet
A. C. Raga, B. Reipurth, A. Esquivel +9
We describe a new method for determining proper motions of extended objects, and a pipeline developed for the application of this method. We then apply this method to an analysis o…
Photo-ionization of planetary winds: case study HD209458b
E. M. Schneiter, A. Esquivel, C. S. Villarreal D'Angelo +3
Close-in hot Jupiters are exposed to a tremendous photon flux that ionizes the neutral escaping material from the planet leaving an observable imprint that makes them an interestin…
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…