Zobrazeno 1 - 10
of 42
pro vyhledávání: '"A. Moranchel-Basurto"'
We study the star-disc interaction in the presence of the strong magnetic field ($B_\star=6.2kG$) of a slowly rotating star. This situation describes a post-merger of the spectral type B and has not been previously investigated. We perform a set of r
Externí odkaz:
http://arxiv.org/abs/2402.00720
2.5-MHD models of circumstellar discs around FS~CMa post-mergers : I. Non-stationary accretion stage
We investigate the dynamic evolution of gaseous region around FS~CMa post-mergers. Due to the slow rotation of a central B-type star, the dynamics is driven mainly by the magnetic field of the central star. Recent observations have allowed us to set
Externí odkaz:
http://arxiv.org/abs/2306.16073
Supernova (SN) explosions can potentially affect the structure and evolution of circumnuclear disks in active galactic nuclei (AGN). Some previous studies have suggested that a relatively low rate of SN explosions can provide an effective value of al
Externí odkaz:
http://arxiv.org/abs/2011.13877
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
Publikováno v:
Monthly Notices of the Royal Astronomical Society; 3/15/2024, Vol. 528 Issue 4, p7310-7319, 10p
Autor:
Alejandro Esquivel, G. Ares de Parga, Pablo F. Velázquez, Estela Marta Reynoso, Ernesto Matías Schneiter, A. Moranchel-Basurto
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 494:1531-1538
We have performed 3D magnetohydrodynamics (MHD) numerical simulations with the aim of exploring the scenario in which the initial mass distribution of a supernova (SN) explosion is anisotropic. The purpose is to analyse if this scenario can also expl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8ee2fae0172689143fad97ebc0182b3e
https://doi.org/10.1093/mnras/staa627
https://doi.org/10.1093/mnras/staa627
Akademický článek
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Akademický článek
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Publikováno v:
The Astrophysical Journal. 906:15
Supernova (SN) explosions can potentially affect the structure and evolution of circumnuclear disks in active galactic nuclei (AGN). Some previous studies have suggested that a relatively low rate of SN explosions can provide an effective value of al
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aeb5403f03bd7f209b48e6e03bfa6f64
https://doi.org/10.3847/1538-4357/abca88
https://doi.org/10.3847/1538-4357/abca88