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/

  • Spatially-resolved stellar population properties of galaxies in voids with the CAVITY project
    Galaxies in voids have been found to be of a later type, bluer, less massive, and to have a slower evolution than galaxies in denser environments (filaments and walls). However, the effect of the void environment on their stellar population properties is still unclear. We aim to address this question using 118 optical integral field unit datacubes
    Conrado, A. et al.

    Advertised on:

    5
    2025
    Citations
    0
  • Size and shape of the trans-Neptunian object (470316) 2007 OC10: Comparison with thermal data
    Context. The shapes of only 12 trans-Neptunian objects have been directly measured, offering crucial insights into their internal structure. These properties are strongly connected to the processes that shaped the early Solar System, and provide important clues about its evolution. Aims. The aim of the present work is to characterise the size
    Gómez-Limón, J. M. et al.

    Advertised on:

    5
    2025
    Citations
    0
  • Signature of spin-down stalling in stellar magnetic activity: The case of the open cluster NGC 6811
    Context. Stellar rotation and magnetic activity have a complex evolution that reveals multiple regimes. One of the related transitions that is seen in the rotation distribution for main-sequence (MS) solar-like stars has been attributed to core-envelope coupling and the consequent angular-momentum transfer between a fast core and a slow envelope
    Santos, A. R. G. et al.

    Advertised on:

    5
    2025
    Citations
    0
  • Searching for R-process-enhanced Stars in the LAMOST Survey. II. Two New r-II Stars in the Milky Way Disk
    R-process-enhanced (RPE) stars are rare and typically metal-poor ([Fe/H] < ‑1.0), primarily found in the Milky Way halo system and dwarf galaxies. This study reports the discovery of two relatively bright, highly RPE stars ([Eu/Fe] > +0.70) located in the Milky Way disk, with [Fe/H] of ‑0.34 and ‑0.80, respectively. These two stars are selected
    Xie, Xiao-Jin et al.

    Advertised on:

    5
    2025
    Citations
    0
  • Revisiting the globular clusters of NGC 1052-DF2
    The ultra-diffuse galaxy (UDG) NGC 1052-DF2 has captured the interest of astronomers ever since the low velocity dispersion measured from ten globular clusters (GCs) suggested a low dark matter fraction. Also, its GC system was found to be unusually bright, with a GC luminosity function peak at least one magnitude brighter than expected for a
    Fahrion, K. et al.

    Advertised on:

    5
    2025
    Citations
    0
  • Red giant evolutionary status determination: The complete Kepler catalog
    Context. Evolved cool stars have three distinct evolutionary status: shell-hydrogen burning (RGB), core-helium and shell-hydrogen burning (RC), and double-shell burning (AGB). Asteroseismology can distinguish between the RC and the other status, but distinguishing RGB and AGB has been difficult seismically and spectroscopically. The precise
    Vrard, M. et al.

    Advertised on:

    5
    2025
    Citations
    0