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pro vyhledávání: '"ROY, J. C."'
Autor:
Villagran, Marco A., Gómez, D. O., Velázquez, P. F., Meyer, D. M. -A., Chiotellis, A., Raga, A. C., Esquivel, A., Toledo-Roy, J. C., Vargas-Rojas, K. M., Schneiter, E. M.
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 progenitor throughout its life. They display a large variety of non-s
Externí odkaz:
http://arxiv.org/abs/2309.16410
Autor:
Velazquez, P. F., Meyer, D. M. -A., Chiotellis, A., Cruz-Alvarez, A. E., Schneiter, E. M., Toledo-Roy, J. C., Reynoso, E. M., Esquivel, A.
Thermonuclear and core-collapse supernova remnants (SNRs) are the nebular leftovers of defunct stars. Their morphology and emission properties provide insights into the evolutionary history of the progenitor star. But while some SNRs are spherical, a
Externí odkaz:
http://arxiv.org/abs/2301.03660
Autor:
Meyer, D. M. -A., Velazquez, P. F., Petruk, O., Chiotellis, A., Pohl, M., Camps-Farina, F., Petrov, M., Reynoso, E. M., Toledo-Roy, J. C., Schneiter, E. M., Castellanos-Ramirez, A., Esquivel, A.
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 properties depend both on the surrounding circumstellar structure shaped by
Externí odkaz:
http://arxiv.org/abs/2206.14495
Akademický článek
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Autor:
Moranchel-Basurto, A., Velázquez, P. F., Giacani, E., Toledo-Roy, J. C., Schneiter, E. M., De Colle, F., Esquivel, A.
In the present work we have modeled the supernova remnant (SNR) G296.5+10, by means of 3D magnetohydrodynamics (MHD) simulations. This remnant belongs to the bilateral SNR group and has an additional striking feature: the rotation measure (RM) in its
Externí odkaz:
http://arxiv.org/abs/1709.00460
Autor:
Velázquez, P. F., Schneiter, E. M., Reynoso, E. M., Esquivel, A., De Colle, F., Toledo-Roy, J. C., Gómez, D. O., Sieyra, M. V., Moranchel-Basurto, A.
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 simulations consider that the remnant expands into a turbulent interstella
Externí odkaz:
http://arxiv.org/abs/1701.05589
Autor:
Castellanos-Ramirez, A., Rodriguez-Gonzalez, A., Esquivel, A., Toledo-Roy, J. C., Olivares, J., Velazquez, P. F.
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 expands into their surrounding medium, shocking it and forming structures
Externí odkaz:
http://arxiv.org/abs/1504.02820
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 618. 3D hydrodynamical simulations of a precessing jet launched from
Externí odkaz:
http://arxiv.org/abs/1408.4699
Akademický článek
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