Publications

This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..

It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/

  • The Large Magellanic Cloud stellar content with SMASH. I. Assessing the stability of the Magellanic spiral arms
    The Large Magellanic Cloud (LMC) is the closest and most studied example of an irregular galaxy. Among its principal defining morphological features, its off-centred bar and single spiral arm stand out, defining a whole family of galaxies known as the Magellanic spirals (Sm). These structures are thought to be triggered by tidal interactions and
    Ruiz-Lara, T. et al.

    Advertised on:

    7
    2020
    Citations
    28
  • The intra-cluster light as a tracer of the total matter density distribution: a view from simulations
    By using deep observations of clusters of galaxies, it has been recently found that the projected stellar mass density closely follows the projected total (dark and baryonic) mass density. In this work, we aim to test these observations using the Cluster-EAGLE simulations. We find that the shape of the stellar mass distribution follows that of the
    Alonso Asensio, I. et al.

    Advertised on:

    7
    2020
    Citations
    0
  • The Impact of the Mass Spectrum of Lenses in Quasar Microlensing Studies. Constraints on a Mixed Population of Primordial Black Holes and Stars
    We show that quasar microlensing magnification statistics induced by a population of point microlenses distributed according to a mass-spectrum can be very well approximated by that of a single-mass, "monochromatic", population. When the spatial resolution (physically defined by the source size) is small as compared with the Einstein radius, the
    Esteban-Gutiérrez, A. et al.

    Advertised on:

    7
    2020
    Citations
    0
  • The impact of strong recombination on temperature determination in planetary nebulae
    The long-standing difference in chemical abundances determined from optical recombination lines and collisionally excited lines raises questions about our understanding of atomic physics, as well as the assumptions made when determining physical conditions and chemical abundances in astrophysical nebulae. Here, we study the recombination
    Gomez-Llanos, V. et al.

    Advertised on:

    7
    2020
  • The impact of strong recombination on temperature determination in planetary nebulae
    The long-standing difference in chemical abundances determined from optical recombination lines and collisionally excited lines raises questions about our understanding of atomic physics, as well as the assumptions made when determining physical conditions and chemical abundances in astrophysical nebulae. Here, we study the recombination
    Gómez-Llanos, V. et al.

    Advertised on:

    7
    2020
    Citations
    13
  • The IACOB spectroscopic database. New interface and second data release
    After almost 12 years gathering data with the 2.56-m Nordic Optical Telescope and the 1.2-m Mercator telescope, the IACOB project has broken the record of compiling high quality, multi-epoch, optical spectra for more than 1000 Northern Galactic O- and B-type stars. To celebrate this important milestone, in this contribution to the first virtual
    Simón-Díaz, S. et al.

    Advertised on:

    7
    2020
    Citations
    9