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/

  • Characterisation of local halo building blocks: Thamnos and Sequoia
    Context. A crucial aspect of galaxy evolution is the pace at which galaxies build up their mass. We can investigate this hierarchical assembly by uncovering and timing accretion events experienced by our Galaxy. Aims. In the Milky Way, accreted debris has been previously identified in the local halo, thanks to the advent of Gaia data. We aim to
    Dodd, Emma et al.

    Advertised on:

    6
    2025
    Citations
    8
  • 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.

    Advertised on:

    6
    2025
    Citations
    2
  • 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.

    Advertised on:

    6
    2025
    Citations
    12
  • 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.

    Advertised on:

    6
    2025
    Citations
    6
  • 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.

    Advertised on:

    6
    2025
    Citations
    12
  • 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.

    Advertised on:

    6
    2025
    Citations
    10