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..

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  • Is the nitrogen-rich source PN K4-47 a true planetary nebula?
    Context. The object K4-47 is a young planetary nebula that exhibits low-ionisation structures in the form of two 'lobes'. The unusual chemistry of the nebula has raised questions about whether K4-47 is a true planetary nebula or if the origins are more exotic in nature. Aims. We aim to investigate the spatially resolved structure of the nebula
    Steinmetz, T. et al.

    Fecha de publicación:

    6
    2026
    Número de citas
    0
  • Investigation of Transit Timing and an Optical Transmission Spectrum of the Hot Jupiter WASP-11 b
    WASP-11 b/HAT-P-10 b is an inflated hot Jupiter, which has a low density that makes it a good target for atmospheric studies using the transmission spectroscopy technique. In this work, we present 31 new transit light curves of WASP-11 b/HAT-P-10 b, obtained through the Spectroscopy and Photometry of Exoplanet Atmospheres Research Network. These
    A-thano, Napaporn et al.

    Fecha de publicación:

    6
    2026
    Número de citas
    0
  • Inferring stellar metallicity and elemental abundances from kinematic and spectroscopic data using machine learning: Implications for exoplanet host stars
    Context. Elemental abundances of FGK stars can be derived routinely from high-resolution optical spectra, but this remains considerably more difficult for cooler stars. Even estimates of the chemical composition of planet-host stars are central for studies of planet formation and interior composition, however. Machine-learning methods offer a
    Adibekyan, V. et al.

    Fecha de publicación:

    6
    2026
    Número de citas
    0
  • Hierarchical assembly in action: A galaxy tail from a disrupting group in the Virgo cluster outskirts
    Context. Group environments are thought to play a key role in shaping galaxy evolution prior to cluster accretion. However, direct observational evidence linking group─cluster interactions to the transformation of low-mass galaxies remains scarce. Aims. The nature and origin of the W cloud, located in the southern outskirts of the Virgo cluster
    Aguerri, J. Alfonso L. et al.

    Fecha de publicación:

    6
    2026
    Número de citas
    0
  • Height Variations of Magnetoacoustic Cutoff Frequency in the Solar Atmosphere
    The determination of the cutoff frequency in real solar observations under different local physical conditions is an important and underexplored aspect of waves in solar physics. This work utilizes the near ultraviolet (NUV) spectrum of the quiet sun (QS), observed by the Interface Region Imaging Spectrograph (IRIS) on November 16th, 2013, in sit
    Kayshap, Pradeep et al.

    Fecha de publicación:

    6
    2026
    Número de citas
    0
  • H I-bearing dark galaxy predictions from constrained Local Group simulations: How many and where to find them
    Context. Dark galaxies are small, dark matter-dominated haloes whose gas remains in hydrostatic and thermal equilibrium and has never formed stars. These systems are of particular interest because they represent a strong prediction of the Lambda cold dark matter (ΛCDM) model. As of today, only a few dark galaxy candidates have been detected so far
    García-Bethencourt, Guacimara et al.

    Fecha de publicación:

    6
    2026
    Número de citas
    5