299 citations · 407 across the 5 of their papers we have counts for
5 papers
Origin of the bilateral structure of the supernova remnant G296.5+10
A. Moranchel-Basurto, P. F. Velázquez, E. Giacani +4
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 an…
A 3D MHD simulation of SN 1006: a polarized emission study for the turbulent case
P. F. Velázquez, E. M. Schneiter, E. M. Reynoso +6
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 simu…
Benchmarking the power of amateur observatories for TTV exoplanets detection
Roman V. Baluev, Evgenii N. Sokov, Vakhit Sh. Shaidulin +13
We perform an analysis of ~80000 photometric measurements for the following 10 stars hosting transiting planets: WASP-2, -4, -5, -52, Kelt-1, CoRoT-2, XO-2, TrES-1, HD 189733, GJ 4…
A ring system detected around the Centaur (10199) Chariklo
F. Braga-Ribas, B. Sicardy, J. L. Ortiz +61
Until now, rings have been detected in the Solar System exclusively around the four giant planets. Here we report the discovery of the first minor-body ring system around the Centa…
3D MHD simulation of flare supra-arcade downflows in a turbulent current sheet medium
M. Cécere, E. Zurbriggen, A. Costa +1
Supra-arcade downflows (SADs) are sunward, generally dark, plasma density depletions originated above posteruption flare arcades. In this paper using 3D MHD simulations we investig…