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

  • Calibrating HMI Magnetograms Using an End-to-end Magnetograph Model
    Numerous solar and space science and operations projects rely heavily on accurate, consistent magnetic field measurements from the solar surface. These projects are hindered by well-known but poorly understood discrepancies between magnetograms obtained with different solar telescopes and instrumentation. Existing efforts to characterize these
    Petrie, Gordon J. D. et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    0
  • Binarity at LOw Metallicity (BLOeM): The multiplicity properties and evolution of BAF-type supergiants
    Given the uncertain evolutionary status of blue supergiant stars, their multiplicity properties hold vital clues to better understand their origin and evolution. As part of The Binarity at LOw Metallicity (BLOeM) campaign in the Small Magellanic Cloud, we present a multi-epoch spectroscopic survey of 128 supergiant stars of spectral type B5–F5
    Patrick, L. R. et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    0
  • Binarity at LOw Metallicity (BLOeM): Multiplicity of early B-type supergiants in the Small Magellanic Cloud
    Context. The blue supergiant (BSG) domain contains a large variety of stars whose past and future evolutionary paths are still highly uncertain. Since binary interaction plays a crucial role in the fate of massive stars, investigating the multiplicity among BSGs helps shed light on the fate of such objects. Aims. We aim to estimate the binary
    Britavskiy, N. et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    0
  • Binarity at LOw Metallicity (BLOeM): Enhanced multiplicity of early B-type dwarfs and giants at Z = 0.2 Z<SUB>⊙</SUB>
    Early B-type stars with initial masses between 8 and 15 M ⊙ are frequently found in multiple systems, as is evidenced by multi-epoch spectroscopic campaigns in the Milky Way and the Large Magellanic Cloud (LMC). Previous studies have shown no strong metallicity dependence in the close-binary (a < 10 au) fraction or orbital-period distributions
    Villaseñor, J. I. et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    0
  • Bar ages derived for the first time in nearby galaxies: Insights into secular evolution from the TIMER sample
    Once galaxies settle their discs and become self-gravitating, stellar bars can form, driving the subsequent evolution of their host galaxy. Determining the ages of bars can therefore shed light on the epoch of the onset of secular evolution. For this work we applied the first broadly applicable methodology to derive bar ages to a sample of 20
    de Sá-Freitas, Camila et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    0
  • ASASSN–14dx: a cataclysmic variable harbouring a massive pulsating white dwarf
    We present the results of our study of ASASSN–14dx, a previously known but poorly characterized cataclysmic variable (CV). The source was observed as part of an ongoing high-time-resolution photometric survey of CVs, which revealed that, in addition to the known 82.8-min orbital period, it also exhibits other transient periods, the strongest of
    Hakala, Pasi et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    0