4 papers
Type I X-Ray Burst Models With Rotation
David Martin, Jordi Jose
Type I X-ray bursts are powered by unstable thermonuclear burning on the surface of accreting neutron stars in close binary systems. These brief X-ray flashes, with light curves fe…
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…
Hydrodynamic simulations of the recurrent nova T Coronae Borealis: Nucleosynthesis predictions
Jordi Jose, Margarita Hernanz
T Coronae Borealis (T CrB) is one of the eleven known recurrent novae in our Galaxy. It was observed in outburst in 1866 and 1946, with additional likely eruptions recorded in 1217…
High-Resolution Simulations of the Interaction Between the Nova/Supernova Ejecta and the Accretion Disk
Axel S. Lechuga, Domingo GarcÃa-Senz, Jordi José
Many nova and type Ia supernova explosion scenarios involve accretion disks. However, direct numerical simulations of these explosive phenomena have barely addressed the question o…