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

  • The Hydrangea simulations: galaxy formation in and around massive clusters
    We introduce the Hydrangea simulations, a suite of 24 cosmological hydrodynamic zoom-in simulations of massive galaxy clusters (M200c = 1014-1015.4 M⊙) with baryon particle masses of ˜106 M⊙. Designed to study the impact of the cluster environment on galaxy formation, they are a key part of the `Cluster-EAGLE' project. They use a galaxy formation
    Bahé, Y. M. et al.

    Fecha de publicación:

    10
    2017
    Número de citas
    180
  • The hypergiant HR 8752 evolving through the yellow evolutionary void
    Context. We study the time history of the yellow hypergiant HR 8752 based on high-resolution spectra (1973-2005), the observed MK spectral classification data, B - V- and V-observations (1918-1996) and yet earlier V-observations (1840-1918). Aims: Our local thermal equilibrium analysis of the spectra yields accurate values of the effective
    Nieuwenhuijzen, H. et al.

    Fecha de publicación:

    10
    2012
    Número de citas
    24
  • The hypnotic dance of Patroclus and Menoetius: Ground-based observations of their 2017-2018 mutual event season.
    Trojans are a significant portion of the small bodies population located within two clouds in the L4 and L5 Lagrangian points of Jupiter's orbit. The study of primitive small bodies is relevant to the origin and nature of volatile and organic material in the early Solar System. Dedicated studies of the nature of these bodies can significantly
    Pinilla-Alonso, Noemí et al.

    Fecha de publicación:

    10
    2018
    Número de citas
    0
  • The IACOB project. II. On the scatter of O-dwarf spectral type - effective temperature calibrations
    Context. We are now in an era of large spectroscopic surveys of OB-type stars. Quantitative spectroscopic analysis of these modern datasets is enabling us to review the physical properties of blue massive stars with robust samples, not only revisiting mean properties and general trends, but also incorporating information about the effects of second
    Simón-Díaz, S. et al.

    Fecha de publicación:

    10
    2014
    Número de citas
    25
  • The imaging magnetograph eXperiment for the SUNRISE balloon Antarctica project
    The SUNRISE balloon project is a high-resolution mission to study solar magnetic fields able to resolve the critical scale of 100 km in the solar photosphere, or about one photon mean free path. The Imaging Magnetograph eXperiment (IMaX) is one of the three instruments that will fly in the balloon and will receive light from the 1m aperture
    Martinez Pillet, Valentin et al.

    Fecha de publicación:

    10
    2004
    Número de citas
    23
  • The impact from survey depth and resolution on the morphological classification of galaxies
    We consistently analyse for the first time the impact of survey depth and spatial resolution on the most used morphological parameters for classifying galaxies through non-parametric methods: Abraham and Conselice-Bershady concentration indices, Gini, M20 moment of light, asymmetry, and smoothness. Three different non-local data sets are used
    Quintana, J. M. et al.

    Fecha de publicación:

    10
    2015
    Número de citas
    19