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/

  • Disc galaxies are still settling. Discovery of the smallest nuclear discs and their young stellar bars
    When galactic discs settle and become massive enough, they are able to form stellar bars. These non-axisymmetric structures induce shocks in the gas, causing it to flow to the centre where nuclear structures, such as nuclear discs and rings, are formed. Previous theoretical and observational studies have hinted at the co-evolution of bars and
    de Sá-Freitas, Camila et al.

    Advertised on:

    10
    2023
    Citations
    3
  • Large Photospheric Doppler Shift in Solar Active Region 12673: I. Field-Aligned Flows
    Delta (δ) sunspots sometimes host fast photospheric flows along the central magnetic polarity inversion line (PIL). Here we study the strong Doppler shift signature in the δ-penumbral light bridge of solar active region NOAA 12673. Observations from the Helioseismic and Magnetic Imager (HMI) indicate highly sheared, strong magnetic fields. Large
    Liu, Jiayi et al.

    Advertised on:

    10
    2023
    Citations
    0
  • Oxygen, sulfur, and iron radial abundance gradients of classical Cepheids across the Galactic thin disk★★★
    Context. Classical Cepheids (CCs) are solid distance indicators and tracers of young stellar populations. Dating back to the beginning of the 20th century, they have been safely adopted to trace the rotation, kinematics, and chemical enrichment history of the Galactic thin disk. Aims: The main aim of this investigation is to provide iron, oxygen
    da Silva, R. et al.

    Advertised on:

    10
    2023
    Citations
    10
  • Refining the properties of the TOI-178 system with CHEOPS and TESS
    Context. The TOI-178 system consists of a nearby late K-dwarf transited by six planets in the super-Earth to mini-Neptune regime, with radii ranging from ~1.1 to 2.9 R ⊕ and orbital periods between 1.9 and 20.7 days. All planets but the innermost one form a chain of Laplace resonances. Mass estimates derived from a preliminary radial velocity (RV)
    Delrez, L. et al.

    Advertised on:

    10
    2023
    Citations
    6
  • The impact of the Large Magellanic Cloud on dark matter direct detection signals
    We study the effect of the Large Magellanic Cloud (LMC) on the dark matter (DM) distribution in the Solar neighborhood, utilizing the Auriga magneto-hydrodynamical simulations of Milky Way (MW) analogues that have an LMC-like system. We extract the local DM velocity distribution at different times during the orbit of the LMC around the MW in the
    Smith-Orlik, Adam et al.

    Advertised on:

    10
    2023
    Citations
    12
  • The [CII] 158 μm emission line as a gas mass tracer in high redshift quiescent galaxies
    A great deal of effort has been made in recent years to probe the gas fraction evolution of massive quiescent galaxies (QGs); however, a clear picture has not yet been established. Recent spectroscopic confirmations at z > 3 offer the chance to measure the residual gas reservoirs of massive galaxies a few hundred Myr after their death and to study
    D'Eugenio, C. et al.

    Advertised on:

    10
    2023
    Citations
    5