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/

  • Serial nominations for the AWH initiative: The paradigm of seven-stone antas and beyond
    In this short report we examine the ideal status of the seven-stone antas (a type of very ancient megalithic monument in the southwest of the Iberian Peninsula) as an excellent candidate for a serial nomination within the Astronomy and World Heritage Initiative. This case will be compared with an extraordinary set of dolmens at the other side of
    Belmonte, Juan Antonio et al.

    Advertised on:

    10
    2016
    Citations
    0
  • Shape, size, physical properties and nature of low-perihelion near-Earth asteroid (3200) Phaethon
    We apply the convex inversion method to the new optical data obtained by six instruments together with the already existing observations and derive convex shape model of low-perihelion near-Earth asteroid (3200) Phaethon. This shape model is then used as an input for the thermophysical modeling. We present new convex shape model and rotational
    Hanus, Josef et al.

    Advertised on:

    10
    2016
    Citations
    1
  • SHARDS: A Global View of the Star Formation Activity at z ~ 0.84 and z ~ 1.23
    In this paper, we present a comprehensive analysis of star-forming galaxies (SFGs) at intermediate redshifts (z ∼ 1). We combine the ultra-deep optical spectro-photometric data from the Survey for High-z Absorption Red and Dead Sources (SHARDS) with deep UV-to-FIR observations in the GOODS-N field. Exploiting two of the 25 SHARDS medium-band
    Cava, A. et al.

    Advertised on:

    10
    2015
    Citations
    17
  • Shear Photospheric Forcing and the Origin of Turbulence in Coronal Loops
    We present a series of numerical simulations aimed at understanding the nature and origin of turbulence in coronal loops in the framework of the Parker model for coronal heating. A coronal loop is studied via reduced magnetohydrodynamic (MHD) simulations in Cartesian geometry. A uniform and strong magnetic field threads the volume between the two
    Rappazzo, A. F. et al.

    Advertised on:

    10
    2010
    Citations
    50
  • Simulating galactic outflows with thermal supernova feedback
    Cosmological simulations make use of sub-grid recipes for the implementation of galactic winds driven by massive stars because direct injection of supernova energy in thermal form leads to strong radiative losses, rendering the feedback inefficient. We argue that the main cause of the catastrophic cooling is a mismatch between the mass of the gas
    Dalla Vecchia, C. et al.

    Advertised on:

    10
    2012
    Citations
    469
  • Simulations of Magnetoacoustic Pulsations in Atmospheres of Rapidly Oscillating Ap Stars
    Rapidly oscillating Ap (roAp) stars exhibit an astrophysically interesting combination of strong, dipolar-like magnetic fields and high-overtone p-mode pulsations similar to the Sun. Recent time-resolved spectroscopy of these stars unravelled a complex picture of propagating magnetoacoustic pulsation waves, with amplitude and phase strongly
    Khomenko, E. et al.

    Advertised on:

    10
    2009
    Citations
    13