3,278 research outputs found

    Building initial models of rotating white dwarfs with SPH

    Get PDF
    A general procedure to build self-gravitational, rotating equilibrium structures with the Smoothed Particle Hydrodynamics (SPH) technique does not exist. In particular, obtaining stable rotating configurations for white dwarf (WD) stars is currently a major drawback of many astrophysical simulations. Rotating WDs with low internal temperatures are connected with both, explosive and implosive scenarios such as type Ia supernova explosions or neutron stars formation. Simulations of these events with SPH codes demand stable enough particle configurations as initial models. In this work we have developed and tested a relaxation method to obtain equilibrium configurations of rotating WDs. This method is straightforward and takes advantage of the excellent mass and angular momentum conservation properties of the SPH technique. Although we focus on rigid rotation and its potential applications to several Type Ia supernova scenarios, we also show that our proposal is also able to provide good initial models in differential rotation, which has the potential to benefit many other types of simulations where rotation plays a capital role, like disk evolution and stellar formation.Peer ReviewedPostprint (published version

    La Constitución apostólica «Ut sit» de 28-XI-1982. Acerca de su «Pars» narrativa.

    Get PDF
    Material incluido en el volumen especial de la revista del Instituto Martín de Azpilcueta, Universidad de Navarra : Ius Canonicum (1999), en honor de Javier Hervada

    La congregación para los obispos

    Get PDF

    El decreto de expulsión del canon 700 y las garantías jurídicas del afectado

    Get PDF

    Los decretos generales de las conferencias episcopales

    Get PDF

    Grid Computing for Fusion Research

    Get PDF
    corecore