Publicaciones

Esta sección ofrece el acceso a la base de datos de Publicaciones que recopila los artículos del IAC publicados en revistas científicas. Por favor, pulsa la flecha del menú para ver todas las opciones de búsqueda y de ordenación de resultados; autor, revista, año, etc..

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  • Polarization Diagnostics of Solar Magnetic Fields
    The solar atmosphere is a highly ionized medium which is the playground of magnetic fields. In the deepest layer (the photosphere), magnetic fields disturb the 'normal' fluid motions forcing the plasma to behave incounterintuitive ways; in the outer layers (the chromosphere and the corona) magnetic fields rule, making the plasma levitate or even
    Manso-Sainz, R.

    Fecha de publicación:

    12
    2011
    Número de citas
    0
  • Polarized Radiation Diagnostics for Measuring the Magnetic Field of the Outer Solar Atmosphere
    The basic idea of optical pumping, for which Alfred Kastler received the 1966 Nobel Prize in physics, is that the absorption and scattering of light that is near-resonant with an optical transition can produce large population imbalances among the magnetic sublevels of atomic ground states as well as in excited states. The degree of this
    Trujillo Bueno, J.

    Fecha de publicación:

    12
    2012
    Número de citas
    0
  • Polarized synchrotron emission in quiescent black hole X-ray transients
    We present near-infrared polarimetric observations of the black hole X-ray binaries Swift J1357.2-0933 and A0620-00. In both sources, recent studies have demonstrated the presence of variable infrared synchrotron emission in quiescence, most likely from weak compact jets. For Swift J1357.2-0933, we find that the synchrotron emission is polarized at
    Russell, D. M. et al.

    Fecha de publicación:

    12
    2016
    Número de citas
    17
  • Position and X-ray Variability of 2A 1704+241
    We present results of analysis of observations of the X-ray source 2A 1704+241 with the Rosat Position Sensitive Proportional Counter (PSPC) and the High Resolution Imager (HRI). 2A 1704+241 was first associated with the M3II star HD154791 (Garcia et al. 1983). The identification, based upon observation with the HEAO 1 SMC and the Einstein IPC, was
    Morgan, W. A., Jr. et al.

    Fecha de publicación:

    12
    1998
    Número de citas
    0
  • Post common envelope binaries from SDSS. XII. The orbital period distribution
    Context. The complexity of the common-envelope phase and of magnetic stellar wind braking currently limits our understanding of close binary evolution. Because of their intrinsically simple structure, observational population studies of white dwarf plus main sequence (WDMS) binaries can potentially test theoretical models and constrain their
    Nebot Gómez-Morán, A. et al.

    Fecha de publicación:

    12
    2011
    Número de citas
    121
  • Post common envelope binaries from SDSS. XIII. Mass dependencies of the orbital period distribution
    Context. Post-common-envelope binaries (PCEBs) consisting of a white dwarf (WD) and a main-sequence secondary star are ideal systems to constrain models of common-envelope (CE) evolution. Until very recently, observed samples of PCEBs have been too small to fully explore this potential, however the recently identified large and relatively
    Zorotovic, M. et al.

    Fecha de publicación:

    12
    2011
    Número de citas
    35