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

  • An updated stellar census of the Quintuplet cluster
    Context. Found within the central molecular zone, the Quintuplet is one of the most massive young clusters in the Galaxy. As a consequence it offers the prospect of constraining stellar formation and evolution in extreme environments. However, current observations suggest that it comprises a remarkably diverse stellar population that is difficult
    Clark, J. S. et al.

    Fecha de publicación:

    10
    2018
    Número de citas
    39
  • Aerosols and Water Ice in Jupiter’s Stratosphere from UV-NIR Ground-based Observations
    Jupiter’s atmosphere has been sounded in transmission from the UV to the IR, as if it were a transiting exoplanet, by observing Ganymede while passing through Jupiter’s shadow. The spectra show strong extinction due to the presence of aerosols and haze in Jupiter’s atmosphere and strong absorption features of methane. Here, we report a new detailed
    López-Puertas, Manuel et al.

    Fecha de publicación:

    10
    2018
    Número de citas
    8
  • A map-making algorithm for the QUIJOTE CMB experiment
    In the last years we obtained a very detailed picture of the Primordial Universe by, among other means, measuring the intensity and the polarization of the Cosmic Microwave Background (CMB). With the last space missions WMAP and Planck we entered in the precision Cosmology era. Nowadays, ground-based experiments are measuring the sky looking for
    Guidi, F. et al.

    Fecha de publicación:

    10
    2018
    Número de citas
    0
  • A collection of model stellar spectra for spectral types B to early-M
    Context. Models of stellar spectra are necessary for interpreting light from individual stars, planets, integrated stellar populations, nebulae, and the interstellar medium. Aims: We provide a comprehensive and homogeneous collection of synthetic spectra for a wide range of atmospheric parameters and chemical compositions. Methods: We compile
    Allende Prieto, C. et al.

    Fecha de publicación:

    10
    2018
    Número de citas
    66
  • A clockwork solution to the flavor puzzle
    We introduce a set of clockwork models of flavor that can naturally explain the large hierarchies of the Standard Model quark masses and mixing angles. Since the clockwork only contains chains of new vector-like fermions without any other dynamical fields, the flavor constraints allow for relatively light new physics scale. For two benchmarks with
    Alonso, R. et al.

    Fecha de publicación:

    10
    2018
    Número de citas
    44
  • 3D non-LTE corrections for Li abundance and 6Li/7Li isotopic ratio in solar-type stars. I. Application to HD 207129 and HD 95456
    Context. Convective motions in solar-type stellar atmospheres induce Doppler shifts that affect the strengths and shapes of spectral absorption lines and create slightly asymmetric line profiles. One-dimensional (1D) local thermodynamic equilibrium (LTE) studies of elemental abundances are not able to reproduce this phenomenon, which becomes
    Harutyunyan, G. et al.

    Fecha de publicación:

    10
    2018
    Número de citas
    24