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

  • AGILE, Fermi, Swift, and GASP/WEBT multi-wavelength observations of the high-redshift blazar 4C +71.07 in outburst
    Context. The flat-spectrum radio quasar 4C +71.07 is a high-redshift (z = 2.172), γ-loud blazar whose optical emission is dominated by thermal radiation from the accretion disc. Aims: 4C +71.07 has been detected in outburst twice by the AGILE γ-ray satellite during the period from the end of October to mid-November 2015, when it reached a γ-ray
    Vercellone, S. et al.

    Fecha de publicación:

    1
    2019
    Número de citas
    9
  • A Second Terrestrial Planet Orbiting the Nearby M Dwarf LHS 1140
    LHS 1140 is a nearby mid-M dwarf known to host a temperate rocky super-Earth (LHS 1140 b) on a 24.737-day orbit. Based on photometric observations by MEarth and Spitzer as well as Doppler spectroscopy from the High Accuracy Radial velocity Planet Searcher, we report the discovery of an additional transiting rocky companion (LHS 1140 c) with a mass
    Ment, K. et al.

    Fecha de publicación:

    1
    2019
    Número de citas
    104
  • A second terrestrial planet orbiting the nearby M dwarf LHS 1140
    LHS 1140 is a nearby mid-M dwarf known to host a temperate rocky super-Earth (LHS 1140 b) on a 24.737-day orbit. Based on photometric observations by MEarth and Spitzer as well as Doppler spectroscopy from HARPS, we present the discovery of an additional transiting rocky companion (LHS 1140 c) with a mass of 1.81 ± 0.39 Earth masses and a radius of
    Ment, K. et al.

    Fecha de publicación:

    1
    2019
    Número de citas
    0
  • A recurrent nova super-remnant in the Andromeda galaxy
    The accretion of hydrogen onto a white dwarf star ignites a classical nova eruption1,2—a thermonuclear runaway in the accumulated envelope of gas, leading to luminosities up to a million times that of the Sun and a high-velocity mass ejection that produces a remnant shell (mainly consisting of insterstellar medium). Close to the upper mass limit of
    Darnley, M. J. et al.

    Fecha de publicación:

    1
    2019
    Número de citas
    36
  • NEUTRON-CAPTURE ELEMENTS IN PLANETARY NEBULAE AS TRACERS OF NUCLEOSYNTHESIS IN AGB STARS
    The main goal of this Thesis is to study the formation of the elements heavier than Fe in asymptotic giant branch (AGB) stars. These elements are formed when iron peak nuclei present in the intershell experience a series of slow neutron-captures and β− decays to form isotopes of heavier elements (the slow neutron-capture process, hereafter s
    Simone Madonna

    Fecha de publicación:

    1
    2019
  • Problems with the dark matter and dark energy hypotheses, and alternative ideas
    Two exotic elements have been introduced into the standard cosmological model: non-baryonic dark matter and dark energy. The success in converting a hypothesis into a solid theory depends strongly on whether we are able to solve the problems in explaining observations with these dark elements and whether the solutions of these problems are unique
    Lopez-Corredoira, Martin

    Fecha de publicación:

    0
    2019
    Número de citas
    4