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

  • Fitting peculiar spectral profiles in He I 10830Å absorption features
    The new generation of solar instruments provides better spectral, spatial, and temporal resolution for a better understanding of the physical processes that take place on the Sun. Multiple-component profiles are more commonly observed with these instruments. Particularly, the He I 10830 Å triplet presents such peculiar spectral profiles, which give
    González Manrique, S. J. et al.

    Fecha de publicación:

    11
    2016
    Número de citas
    18
  • FliPer: A global measure of power density to estimate surface gravities of main-sequence solar-like stars and red giants
    Asteroseismology provides global stellar parameters such as masses, radii, or surface gravities using mean global seismic parameters and effective temperature for thousands of low-mass stars (0.8 M⊙ < M < 3 M⊙). This methodology has been successfully applied to stars in which acoustic modes excited by turbulent convection are measured. Other
    Bugnet, L. et al.

    Fecha de publicación:

    11
    2018
    Número de citas
    29
  • Flow and magnetic field properties in the trailing sunspots of active region NOAA 12396
    Improved measurements of the photospheric and chromospheric three-dimensional magnetic and flow fields are crucial for a precise determination of the origin and evolution of active regions. We present an illustrative sample of multi-instrument data acquired during a two-week coordinated observing campaign in August 2015 involving, among others, the
    Verma, M. et al.

    Fecha de publicación:

    11
    2016
    Número de citas
    5
  • Formation of Fullerenes in H-containing Planetary Nebulae
    Hydrogen depleted environments are considered an essential requirement for the formation of fullerenes. The recent detection of C60 and C70 fullerenes in what was interpreted as the hydrogen-poor inner region of a post-final helium shell flash planetary nebula (PN) seemed to confirm this picture. Here, we present strong evidence that challenges the
    García-Hernández, D. A. et al.

    Fecha de publicación:

    11
    2010
    Número de citas
    157
  • Formation of lithium lines in very cool dwarfs.
    We present LTE and NLTE results on the formation of LiI lines (λ6103, λ6708, and λ8126) in the atmospheres of solar metallicity dwarfs with effective temperatures in the range 5500K to 2000K. NLTE effects are governed by overionization of Li and by the interlocking effects of energy levels. For stars with T_eff_>=4000K, we confirm previous findings
    Pavlenko, Y. V. et al.

    Fecha de publicación:

    11
    1995
    Número de citas
    75
  • Fossil group origins - VI. Global X-ray scaling relations of fossil galaxy clusters
    We present the first pointed X-ray observations of 10 candidate fossil galaxy groups and clusters. With these Suzaku observations, we determine global temperatures and bolometric X-ray luminosities of the intracluster medium (ICM) out to r500 for six systems in our sample. The remaining four systems show signs of significant contamination from non
    Kundert, A. et al.

    Fecha de publicación:

    11
    2015
    Número de citas
    15