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..

Además ofrece acceso al  repositorio de preprints del IAC: https://research.iac.es/preprints/l

  • Slow rupture of an aseismic fault in a seismogenic region of Central Italy
    Slow earthquakes and afterslips prove that the Earth does not have just two response time scales, i.e. that of tectonic loading and that of regular earthquakes. A swarm of slow earthquakes, with time constants of the order of hundreds of seconds, has been detected by a laser interferometer below the Gran Sasso massif (Italy). We analyse and model
    Amoruso, Antonella et al.

    Fecha de publicación:

    12
    2002
    Número de citas
    0
  • Small-scale magnetic flux emergence in a sunspot light bridge
    Context. Light bridges are convective intrusions in sunspots that often show enhanced chromospheric activity. Aims: We seek to determine the nature of flux emergence in a light bridge and the processes related to its evolution in the solar atmosphere. Methods: We analyse a sequence of high-resolution spectropolarimetric observations of a sunspot
    Louis, R. E. et al.

    Fecha de publicación:

    12
    2015
    Número de citas
    28
  • SMASHing the LMC: Mapping a Ring-like Stellar Overdensity in the LMC Disk
    We explore the stellar structure of the Large Magellanic Cloud (LMC) disk using data from the Survey of the MAgellanic Stellar History and the Dark Energy Survey. We detect a ring-like stellar overdensity in the red clump star count map at a radius of ∼6° (∼5.2 kpc at the LMC distance) that is continuous over ∼270° in position angle and is only
    Choi, Y. et al.

    Fecha de publicación:

    12
    2018
    Número de citas
    40
  • SN 2012aa: A transient between Type Ibc core-collapse and superluminous supernovae
    Context. Research on supernovae (SNe) over the past decade has confirmed that there is a distinct class of events which are much more luminous (by 2 mag) than canonical core-collapse SNe (CCSNe). These events with visual peak magnitudes ≲-21 are called superluminous SNe (SLSNe). The mechanism that powers the light curves of SLSNe is still not well
    Roy, R. et al.

    Fecha de publicación:

    12
    2016
    Número de citas
    29
  • Soft X-ray transient light curves as standard candles: exponential versus linear decays
    A recent paper by King & Ritter proposed that the light curves of soft X-ray transients (SXTs) are dominated by the effect of irradiation of the accretion disc by the central X-rays. This prevents the onset of the cooling wave which would otherwise return the disc to the quiescent state, and so prolongs the outbursts beyond those in dwarf nova
    Shahbaz, T. et al.

    Fecha de publicación:

    12
    1998
    Número de citas
    85
  • Solar Abundance Corrections Derived Through Three-dimensional Magnetoconvection Simulations
    We explore the effect of the magnetic field when using realistic three-dimensional convection experiments to determine solar element abundances. By carrying out magnetoconvection simulations with a radiation-hydro code (the Copenhagen stagger code) and through a posteriori spectral synthesis of three Fe I lines, we obtain evidence that moderate
    Fabbian, D. et al.

    Fecha de publicación:

    12
    2010
    Número de citas
    58