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

  • High-resolution Hα imaging of the northern Galactic plane and the IGAPS image database
    The INT Galactic Plane Survey (IGAPS) is the merger of the optical photometric surveys IPHAS and UVEX based on data from the Isaac Newton Telescope (INT) obtained between 2003 and 2018. It captures the entire northern Galactic plane within the Galactic coordinate range |b|< 5° and 30° < ℓ < 215°. From the beginning, the incorporation of narrow-band
    Greimel, R. et al.

    Fecha de publicación:

    11
    2021
    Número de citas
    12
  • Gas and dust from extremely metal-poor AGB stars
    Context. The study of stars that evolve through the asymptotic giant branch (AGB) proves crucial in several astrophysical contexts because these objects provide important feedback to the host system in terms of the gas that is poured into the interstellar medium after being exposed to contamination from nucleosynthesis processes, and in terms of
    Ventura, P. et al.

    Fecha de publicación:

    11
    2021
    Número de citas
    18
  • Gaia-ESO survey: Lithium abundances in open cluster Red Clump stars
    Context. It has recently been suggested that all giant stars with masses below 2 M ⊙ suffer an episode of surface lithium enrichment between the tip of the red giant branch (RGB) and the red clump (RC). Aims: We test if the above result can be confirmed in a sample of RC and RGB stars that are members of open clusters. Methods: We discuss Li
    Magrini, L. et al.

    Fecha de publicación:

    11
    2021
    Número de citas
    25
  • Fossil group origins. XI. The dependence of galaxy orbits on the magnitude gap
    Aims: We aim to study how the orbits of galaxies in clusters depend on the prominence of the corresponding central galaxies. Methods: We divided our data set of ∼100 clusters and groups into four samples based on their magnitude gap between the two brightest members, Δm 12. We then stacked all the systems in each sample in order to create four
    Zarattini, S. et al.

    Fecha de publicación:

    11
    2021
    Número de citas
    10
  • Failed-transition outbursts in black hole low-mass X-ray binaries
    Black hole low-mass X-ray binaries (BH LMXBs) evolve in a similar way during outburst. Based on the X-ray spectrum and variability, this evolution can be divided into three canonical states: low/hard, intermediate, and high/soft state. BH LMXBs evolve from the low/hard to the high/soft state through the intermediate state in some outbursts (here
    Alabarta, K. et al.

    Fecha de publicación:

    11
    2021
    Número de citas
    42
  • Extragalactic Magnetism with SOFIA (Legacy Program). I. The Magnetic Field in the Multiphase Interstellar Medium of M51
    The recent availability of high-resolution far-infrared (FIR) polarization observations of galaxies using HAWC+/SOFIA has facilitated studies of extragalactic magnetic fields in the cold and dense molecular disks. We investigate whether any significant structural differences are detectable in the kiloparsec-scale magnetic field of the grand design
    Borlaff, Alejandro S. et al.

    Fecha de publicación:

    11
    2021
    Número de citas
    32