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

  • Inference of magnetic field strength and density from damped transverse coronal waves
    A classic application of coronal seismology uses transverse oscillations of waveguides to obtain estimates of the magnetic field strength. The procedure requires information on the density of the structures. Often it ignores the damping of the oscillations. We computed marginal posteriors for parameters such as the waveguide density, the density
    Arregui, I. et al.

    Fecha de publicación:

    5
    2019
    Número de citas
    10
  • Homogeneous photometry - VII. Globular clusters in the Gaia era
    We present wide-field, ground-based Johnson-Cousins UBVRI photometry for 48 Galactic globular clusters based on about 90 000 public and proprietary images. The photometry is calibrated with the latest transformations obtained in the framework of our secondary standard project, with typical internal and external uncertainties of order a few
    Stetson, P. B. et al.

    Fecha de publicación:

    5
    2019
    Número de citas
    120
  • Galaxies with monstrous black holes in galaxy cluster environments
    Massive early-type galaxies follow a tight relation between the mass of their central supermassive black hole (MBH) and their stellar mass (M⋆). The origin of observed positive outliers from this relation with extremely high MBH (> 109 M_{⊙ }) remains unclear. We present a study of such outliers in the Hydrangea/C-EAGLE cosmological hydrodynamical
    van Son, Lieke A. C. et al.

    Fecha de publicación:

    5
    2019
    Número de citas
    17
  • Gaia-assisted selection of a quasar reddened by dust in an extremely strong damped Lyman-α absorber at z = 2.226
    Damped Lyman-α absorbers (DLAs) as a class of quasi-stellar object (QSO) absorption-line systems are currently our most important source of detailed information on the cosmic chemical evolution of galaxies. However, the degree to which this information is biased by dust remains to be understood. One strategy is to specifically search for QSOs that
    Geier, S. J. et al.

    Fecha de publicación:

    5
    2019
    Número de citas
    11
  • Fundamental Physics with Brown Dwarfs: The Mass-Radius Relation
    The lowest-mass stars, brown dwarfs and giant exoplanets span a minimum in the mass-radius relationship that probes the fundamental physics of extreme states of matter, magnetism, and fusion. This White Paper outlines scientific opportunities and the necessary resources for modeling and measuring the mass- radius relationship in this regime.
    Burgasser, Adam et al.

    Fecha de publicación:

    5
    2019
    Número de citas
    0
  • From kpcs to the central parsec of NGC 1097: feeding star formation and a black hole at the same time
    A panchromatic view of the star-forming ring and feeding process in the central kpc of the galaxy NGC 1097 is presented. The assembled IR to UV images at ˜10 pc resolution allow us to characterize the population of circa 250 clusters in the ring and disentangle the network of filaments of dust and gas that enshroud and feed them. The ring is a
    Prieto, M. A. et al.

    Fecha de publicación:

    5
    2019
    Número de citas
    28