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

  • 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.

    Fecha de publicación:

    10
    2023
    Número de citas
    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.

    Fecha de publicación:

    10
    2023
    Número de citas
    9
  • 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.

    Fecha de publicación:

    10
    2023
    Número de citas
    3
  • 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.

    Fecha de publicación:

    10
    2023
    Número de citas
    10
  • 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.

    Fecha de publicación:

    10
    2023
    Número de citas
    4
  • Workshop Summary: Exoplanet Orbits and Dynamics
    Exoplanetary systems show a wide variety of architectures, which can be explained by different formation and dynamical evolution processes. Precise orbital monitoring is mandatory to accurately constrain their orbital and dynamical parameters. Although major observational and theoretical advances have been made in understanding the architecture and
    Maire, Anne-Lise et al.

    Fecha de publicación:

    10
    2023
    Número de citas
    0