86 citations · 688 across the 26 of their papers we have counts for
26 papers
Interaction between the ejecta, the accretion disk, and the secondary star in the recurrent nova system U Sco
Joana Figueira, Jordi Jose, Ruben Cabezon +1
Most efforts in the modeling of recurrent novae have centered on the initial phases of the explosion and ejection, overlooking the subsequent interaction of the ejecta, first with…
The neutron star population in M28: a joint Chandra/GBT look at pulsar paradise
Eda Vurgun, Manuel Linares, Scott Ransom +7
We present the results of a deep study of the neutron star (NS) population in the globular cluster M28 (NGC 6626), using the full 330-ks 2002-2015 ACIS dataset from the Chandra X-r…
Conservative, density-based smoothed particle hydrodynamics with improved partition of the unity and better estimation of gradients
Domingo García-Senz, Rubén M. Cabezón, José A. Escartín
The correct evaluation of gradients is at the cornerstone of the smoothed particle hydrodynamics (SPH) technique. Using an integral approach to estimate gradients has proven to enh…
Three-dimensional simulations of the interaction between the nova ejecta, the accretion disk, and the companion star
Joana Figueira, Jordi Jose, Enrique Garcia-Berro +3
Context. Classical novae are thermonuclear explosions hosted by accreting white dwarfs in stellar binary systems. Material piles up on top of the white dwarf star under mildly dege…
SPHYNX: an accurate density-based SPH method for astrophysical applications
Ruben M. Cabezon, Domingo Garcia-Senz, Joana Figueira
Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, an accurate numerical simulation of these phenomena is mandatory to correctly model an…
Gamma-Ray emission from SN2014J near maximum optical light
J. Isern, P. Jean, E. Bravo +17
The optical light curve of Type Ia supernovae (SNIa) is powered by thermalized gamma-rays produced by the decay of 56Ni and 56Co, the main radioactive isotopes synthesized by the t…