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 Origin of Asteroid 162173 (1999 JU3)
    Near-Earth asteroid (162173) 1999 JU3 (henceforth JU3) is a potentially hazardous asteroid and the target of the Japanese Aerospace Exploration Agency’s Hayabusa-2 sample return mission. JU3 is also a backup target for two other sample return missions: NASA’s OSIRIS-REx and the European Space Agency’s Marco Polo-R. We use dynamical information to
    Comfort, Christine et al.

    Fecha de publicación:

    10
    2013
    Número de citas
    0
  • The nature of LINER galaxies:. Ubiquitous hot old stars and rare accreting black holes
    Context. Galaxies, which often contain ionised gas, sometimes also exhibit a so-called low-ionisation nuclear emission line region (LINER). For 30 years, this was attributed to a central mass-accreting supermassive black hole (more commonly known as active galactic nucleus, AGN) of low luminosity, making LINER galaxies the largest AGN sub
    Singh, R. et al.

    Fecha de publicación:

    10
    2013
    Número de citas
    280
  • The Dynamics of the Solar Radiative Zone
    The dynamics of the solar radiative interior are still poorly constrained by comparison to the convective zone. This disparity is even more marked when we attempt to derive meaningful temporal variations. Many data sets contain a small number of modes that are sensitive to the inner layers of the Sun, but we found that the estimates of their
    Eff-Darwich, A. et al.

    Fecha de publicación:

    10
    2013
    Número de citas
    24
  • THE CENTERS OF GALAXIES AT PARSEC SCALES: THE CASE OF M87
    Los centros de las galaxias muestran algunos de los extremos más fascinantes de la naturaleza. Se puede encontrar en ellos: altas concentraciones estelares, agujeros negros supermasivos, altas concentraciones de gas, fuertes campos magnéticos, poblaciones estelares no convencionales, explosiones de formación estelar, etc. Se piensa que estas
    Mireia Montes Quiles

    Fecha de publicación:

    10
    2013
  • The BaSTI Stellar Evolution Database: models for extremely metal-poor and super-metal-rich stellar populations
    We present an extension of the BaSTI (Bag of Stellar Tracks and Isochrones) stellar evolution database to extremely metal-poor (Z = 10-5) and super-metal-rich (Z = 0.05) metallicities, with both scaled-solar and α-enhanced ([α/Fe] = 0.4) heavy element distributions. These new tracks (from the pre-main sequence to the early-asymptotic giant branch
    Pietrinferni, A. et al.

    Fecha de publicación:

    10
    2013
    Número de citas
    72
  • The Ages of 55 Globular Clusters as Determined Using an Improved \Delta V^HB_TO Method along with Color-Magnitude Diagram Constraints, and Their Implications for Broader Issues
    Ages have been derived for 55 globular clusters (GCs) for which Hubble Space Telescope Advanced Camera for Surveys photometry is publicly available. For most of them, the assumed distances are based on fits of theoretical zero-age horizontal-branch (ZAHB) loci to the lower bound of the observed distributions of HB stars, assuming reddenings from
    VandenBerg, D. A. et al.

    Fecha de publicación:

    10
    2013
    Número de citas
    445