Zobrazeno 1 - 10
of 40
pro vyhledávání: '"Fabio D. Lora-Clavijo"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 519:3584-3594
Magnetic fields in black hole accretion disks are associated with processes of mass accretion and energy amplification. The contribution of the magnetic field due to the magnetic polarization of the material induces effects on the physical properties
Autor:
Bridget Ierace, Fabio D. Lora-Clavijo, P. Chris Fragile, Oscar M Pimentel Diaz, Deepika A. Bollimpalli
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 505:4278-4288
The magneto-rotational instability (MRI) is the most likely mechanism for transportation of angular momentum and dissipation of energy within hot, ionized accretion discs. This instability is produced through the interactions of a differentially rota
Existen observaciones que indican que el campo magnético en la atmósfera solar tiene twist, esto cumple un papel muy importante en diferentes fenómenos solares como la reconexión magnética, las fulguraciones solares, entre otros. Sin embargo, su
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::adf4a600db9a3935eb5a032c06dfc6c0
https://repositorio.accefyn.org.co/handle/001/1274
https://repositorio.accefyn.org.co/handle/001/1274
Publikováno v:
Repositório Científico de Acesso Aberto de Portugal
Repositório Científico de Acesso Aberto de Portugal (RCAAP)
instacron:RCAAP
Repositório Científico de Acesso Aberto de Portugal (RCAAP)
instacron:RCAAP
The recent gravitational wave transient GW190521 has been interpreted by the LIGO-Virgo collaboration (LVC) as sourced by a binary black hole (BH) merger. According to the LVC parameter estimation, at least one of these progenitors falls into the so-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7b0275910e15dc1eb813686798c93dec
http://arxiv.org/abs/2101.01705
http://arxiv.org/abs/2101.01705
Autor:
Antonio C. Gutiérrez-Piñeres, J. A. Arrieta-Villamizar, Fabio D. Lora-Clavijo, Oscar M. Pimentel, J. M. Velásquez-Cadavid
One crucial problem in relativistic astrophysics is that of the nature of black hole candidates. It is usually assumed that astrophysical black holes are described by the Schwarzschild or Kerr space-times; however, there is no direct evidence to asse
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f6b557f7a7624055782d35690322d122
http://arxiv.org/abs/2007.13600
http://arxiv.org/abs/2007.13600
Autor:
Cuauhtemoc Campuzano Vargas, Fabio D. Lora-Clavijo, Alejandro Cruz-Osorio, Luis Alejandro García Mora, Griselda Arroyo-Chávez
It is well known that the equation of state (EoS) of compact objects like neutron and quark stars is not determined despite there are several sophisticated models to describe it. From the electromagnetic observations, summarized in \cite{Lattimer01},
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d2a6a4e967ad02125b646d2f52a488a0
We measure the effects of non-isotropic thermal conduction on generation of solar chromospheric jets through numerical simulations carried out with the use of one fluid MHD code MAGNUS. Following the work of Srivastava et al. (2018), we consider the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::df34e56613dede3103b2cefd56e48389
We numerically simulate emergence of a magnetic plasma blob into a solar coronal hole. This blob may be associated with granulation and therefore it has a weak magnetic field. Two-dimensional simulations are performed using the MAGNUS code which solv
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b7109778eacfc64c62bf1643d4ddc3a8
http://arxiv.org/abs/1910.11814
http://arxiv.org/abs/1910.11814
Publikováno v:
European Journal of Physics. 42:065001
In geophysics, wave propagation in elastic media is a crucial subject. In this context, seismology has made significant progress as a result of numerous advances, among these stands out the advancement of numerical methods such as the finite-differen
Publikováno v:
Physics Letters A. 381:563-567
We study the dynamics of the planar circular restricted three-body problem in the context of a pseudo-Newtonian approximation. By using the Fodor-Hoenselaers-Perj\'es procedure, we perform an expansion in the mass potential of a static massive spheri