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

  • Probing Abundance Variations Among Multiple Stellar Populations in the Metal-poor Globular Cluster NGC 2298 Using Gemini-South/GHOST
    Studying the abundances in metal-poor globular clusters is crucial for understanding the formation of the Galaxy and the nucleosynthesis processes in the early Universe. We observed 13 red-giant stars from the metal-poor globular cluster NGC 2298 using the newly commissioned GHOST spectrograph at Gemini South. We derived stellar parameters and
    Bandyopadhyay, Avrajit et al.

    Fecha de publicación:

    7
    2025
    Número de citas
    0
  • Optimizing the analysis of emission lines in galaxies: the case of the MUSE TIMER galaxy NGC 613
    Galaxy evolution is driven by spatially distributed processes with varying time-scales. Integral field spectroscopy provides spatially resolved information about these processes. Nevertheless, disentangling these processes, which are related to both the underlying stellar populations and the interstellar medium can be challenging. We present a case
    Silva-Lima, Luiz A. et al.

    Fecha de publicación:

    7
    2025
    Número de citas
    0
  • INSPIRE: INvestigating Stellar Populations In RElics - IX. KiDS J0842 + 0059: the first fully confirmed relic beyond the local Universe
    Relics are massive, compact and quiescent galaxies that assembled the majority of their stars in the early Universe and lived untouched until today, completely missing any subsequent size growth caused by mergers and interactions. They provide the unique opportunity to put constraints on the first phase of mass assembly in the Universe with the
    Tortora, C. et al.

    Fecha de publicación:

    7
    2025
    Número de citas
    0
  • Is the symbiotic recurrent nova T CrB late? Recent photometric evolution and comparison with past pre-outburst behaviour
    T CrB is a symbiotic recurrent nova that last erupted in 1946. Given its recurrence time-scale of approximately 80 yr, the next outburst is eagerly anticipated by the astronomical community. In this work, we analyse the optical light curves of T CrB, comparing recent photometric evolution with historical data to evaluate potential predictive
    Merc, Jaroslav et al.

    Fecha de publicación:

    7
    2025
    Número de citas
    0
  • A transiting rocky super-Earth and a non-transiting sub-Neptune orbiting the M dwarf TOI-771
    Context. The origin and evolution of the sub-Neptune population is a highly debated topic in the exoplanet community. With the advent of JWST, atmospheric studies can now put unprecedented constraints on the internal composition of this population. In this context, the THIRSTEE project aims to investigate the population properties of sub-Neptunes
    Lacedelli, G. et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    0
  • Accretion Diagnostics for JWST–MIRI: Establishing the Relationship between Mid-Infrared Hydrogen Lines and the Accretion Luminosity
    We have established mid-infrared hydrogen recombination lines observed with JWST as accretion tracers for pre-main-sequence stars that accrete from circumstellar disks. These new relations equip the community with a direct measurement of the accretion luminosity from MIRI-MRS spectra. A MIRI-derived accretion luminosity is fundamental for time
    Tofflemire, Benjamin et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    0