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

  • Mass loss from an extreme OH/IR star: OH 26.5+0.6
    Observations of H2O isotopologues of the extreme OH/IR star OH 26.5+0.6 show that the star has an initial mass consistent with it being an intermediate-mass star. The Herschel-HIFI spectra show clear detection of H216O and H217O while H218O is missing, consistent with the prediction of hot bottom burning which occurs in stars with an initial mass
    Justtanont, K. et al.

    Fecha de publicación:

    2017
    Número de citas
    1
  • MAGIC detection of sub-TEV emission from gravitationally lensed blazar QSO B0218+357
    The blazar QSO B0218+357 is the first gravitationally lensed blazar detected in the very high energy (VHE, E > 100 GeV) gamma-ray spectral range (Ahnen et al. 2016). It is gravitationally lensed by the intervening galaxy B0218+357G (z l = 0.68466 +/- 0.00004, Carilli et al. 1993), which splits the blazar emission into two components, spatially
    Dominis Prester, D. et al.

    Fecha de publicación:

    2017
    Número de citas
    0
  • Exploring circumstellar effects on the Li abundances in massive Galactic AGB stars.
    We have explored the circumstellar effects on the Li abundance determination in a complete sample of O-rich Galactic asymptotic giant branch (AGB) stars, previously studied with hydrostatic models. We use a modified version of the spectral synthesis code Turbospectrum and more realistic extended model atmospheres that consider the presence of a
    Pérez-Mesa, V. et al.

    Fecha de publicación:

    2017
    Número de citas
    0
  • Elusive Accretion Discs in Low Luminosity AGN
    Low luminosity AGN (LLAGN) represent the vast majority of the AGN population in the near universe. However, they show intrinsic differences when compared to the Unified Model scenario, i.e. a lack of both the big blue bump and the IR bump in their spectral energy distribution (SED), which are the signatures of an accretion disk and a torus
    Fernández-Ontiveros, J. A. et al.

    Fecha de publicación:

    2017
    Número de citas
    0
  • Cosmic chemistry from AGB stars and its dependence on the initial stellar mass .
    Asymptotic giant branch (AGB) stars synthetise a variety of elements in their deep hot layers, mix them to the stellar surface, and shed them into their surrounding by stellar winds. Through this series of processes (nucleosynthesis, mixing, and winds) they contribute to the chemical evolution of stellar groups and galaxies. Specifically, they
    Lugaro, M. et al.

    Fecha de publicación:

    2017
    Número de citas
    0
  • Atmospheric Monitoring at the Site of the MAGIC Telescopes
    The MAGIC telescopes in La Palma, Canary Islands, measure the Cherenkov light emitted by gamma ray-induced extended air showers in the atmosphere. The good knowledge of the atmospheric parameters is important, both for the correct and safe operations of the telescopes, but also for subsequent data analysis. A weather station measures the state
    Will, M.

    Fecha de publicación:

    2017
    Número de citas
    2