Publications

This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..

It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/

  • 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.

    Advertised on:

    12
    2002
    Citations
    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.

    Advertised on:

    12
    2015
    Citations
    27
  • 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.

    Advertised on:

    12
    2016
    Citations
    27
  • 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.

    Advertised on:

    12
    1998
    Citations
    84
  • 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.

    Advertised on:

    12
    2010
    Citations
    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.

    Advertised on:

    12
    2012
    Citations
    43