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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  • 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
  • Solar Fe abundance and magnetic fields. Towards a consistent reference metallicity
    Aims: We investigate the impact on Fe abundance determination of including magnetic flux in series of 3D radiation-magnetohydrodynamics (MHD) simulations of solar convection, which we used to synthesize spectral intensity profiles corresponding to disc centre. Methods: A differential approach is used to quantify the changes in theoretical
    Fabbian, D. et al.

    Fecha de publicación:

    12
    2012
    Número de citas
    43
  • Solar irradiance, cosmic rays and cloudiness over daily timescales
    Although over centennial and greater timescales solar variability may be one of the most influential climate forcing agents, the extent to which solar activity influences climate over shorter time periods is poorly understood. If a link exists between solar activity and climate, it is likely via a mechanism connected to one (or a combination) of
    Laken, B. A. et al.

    Fecha de publicación:

    12
    2011
    Número de citas
    11