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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  • 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
  • Design of an adaptable Stokes polarimeter for exploring chromospheric magnetism
    The chromosphere is a highly complex and dynamic layer of the Sun, that serves as a conduit for mass and energy supply between two, very distinct regions of the solar atmosphere, namely, the photosphere and corona. Inferring magnetic fields in the chromosphere, has thus become an important topic, that can be addressed with large-aperture solar
    Louis, R. E. et al.

    Fecha de publicación:

    10
    2017
    Número de citas
    0
  • Comparison of Solar Fine Structure Observed Simultaneously in Lyα and Mg ii h
    The Chromospheric Lyman Alpha Spectropolarimeter (CLASP) observed the Sun in H i Lyα during a suborbital rocket flight on 2015 September 3. The Interface Region Imaging Telescope (IRIS) coordinated with the CLASP observations and recorded nearly simultaneous and co-spatial observations in the Mg ii h and k lines. The Mg ii h and Lyα lines are
    Schmit, D. et al.

    Fecha de publicación:

    10
    2017
    Número de citas
    8
  • Close binary central stars and the abundance discrepancy - new extreme objects
    Recent work (Corradi et al. 2015; Jones et al. 2016) has shown that the phenomenon of extreme abundance discrepancies, where recombination line abundances exceed collisionally excited line abundances by factors of 10 or more, seem to be strongly associated with planetary nebulae with close binary central stars. To further investigate, we have
    Wesson, R. et al.

    Fecha de publicación:

    10
    2017
    Número de citas
    8
  • Chemical abundances of 1111 FGK stars from the HARPS GTO planet search program. II. Cu, Zn, Sr, Y, Zr, Ba, Ce, Nd, and Eu
    Aims: To understand the formation and evolution of the different stellar populations within our Galaxy it is essential to combine detailed kinematical and chemical information for large samples of stars. The aim of this work is to explore the chemical abundances of neutron capture elements which are a product of different nucleosynthesis processes
    Delgado Mena, E. et al.

    Fecha de publicación:

    10
    2017
    Número de citas
    178
  • Central Stars of Planetary Nebulae
    In this brief invited review, I will attempt to summarise some of the key areas of interest in the study of central stars of planetary nebulae which (probably) will not be covered by other speakers' proceedings. The main focus will, inevitably, be on the subject of multiplicity, with special emphasis on recent results regarding triple central star
    Jones, D.

    Fecha de publicación:

    10
    2017
    Número de citas
    7