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

  • Imaging the elusive H-poor gas in planetary nebulae with large abundance discrepancy factors
    The discrepancy between abundances computed using optical recombination lines (ORLs) and collisionally excited lines (CELs) is a major, unresolved problem with significant implications for the determination of chemical abundances throughout the Universe. In planetary nebulae (PNe), the most common explanation for the discrepancy is that two
    García-Rojas, J. et al.

    Fecha de publicación:

    10
    2017
    Número de citas
    10
  • Hunting for binary central stars of planetary nebulae: exploiting archival data
    The detection of new binary central stars of planetary nebulae is crucial to definitively determine the importance of binary interactions in the nebular morphology. In this context, we are working on a project that aims to increase the low number of binary central stars detected so far. For that, we are first analyzing public archival data in order
    Aller, A. et al.

    Fecha de publicación:

    10
    2017
    Número de citas
    0
  • GTC/CanariCam mid-IR imaging of the fullerene-rich planetary nebula IC 418
    The formation process(es) of fullerenes in space is still uncertain and several mechanisms have been proposed in the literature. In particular, the most accepted idea to explain the simultaneous presence of fullerenes and PAH-like emission in the H-rich circumstellar envelopes of PNe is that these molecular species may be formed from the
    Díaz-Luis, J. J. et al.

    Fecha de publicación:

    10
    2017
    Número de citas
    0
  • Flows along arch filaments observed in the GRIS `very fast spectroscopic mode'
    A new generation of solar instruments provides improved spectral, spatial, and temporal resolution, thus facilitating a better understanding of dynamic processes on the Sun. High-resolution observations often reveal multiple-component spectral line profiles, e.g., in the near-infrared He i 10830 Å triplet, which provides information about the
    González Manrique, S. J. et al.

    Fecha de publicación:

    10
    2017
    Número de citas
    5
  • Flare activity and photospheric analysis of Proxima Centauri
    Context. We present the analysis of emission lines in high-resolution optical spectra of the planet-host star Proxima Centauri (Proxima) classified as a M5.5V. Aims: We carry out a detailed analysis of the observed spectra to get a better understanding of the physical conditions of the atmosphere of this star. Methods: We identify the emission
    Pavlenko, Y. et al.

    Fecha de publicación:

    10
    2017
    Número de citas
    19
  • Disproving the validated planets K2-78b, K2-82b, and K2-92b. The importance of independently confirming planetary candidates
    Context. Transiting super-Earths orbiting bright stars in short orbital periods are interesting targets for the study of planetary atmospheres. Aims: While selecting super-Earths suitable for further characterisation from the ground from a list of confirmed and validated exoplanets detected by K2, we found some suspicious cases that led to us
    Cabrera, J. et al.

    Fecha de publicación:

    10
    2017
    Número de citas
    31