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

  • On the action of UV photons on hydrogenated fulleranes C60H36 and C60D36

    Fulleranes, the hydrogenated fullerenes C60H36 and C60D36 have been synthesized in n-hexane where they show an absorption maximum at 217 nm in their electronic absorption spectra with molar extinction coefficients ɛ217 = 17140 and 16480L cm-1 mol-1, respectively, which correspond to absorption cross-sections of order 6500 Mbarn, about 10 times

    Cataldo, Franco et al.

    Fecha de publicación:

    11
    2009
    Número de citas
    44
  • On the Central Helium-burning Variable Stars of the LeoI Dwarf Spheroidal Galaxy

    We present a study of short-period, central helium-burning variable stars in the Local Group dwarf spheroidal galaxy LeoI, including 106 RR Lyrae stars and 51 Cepheids. So far, this is the largest sample of Cepheids and the largest Cepheids to RR Lyrae ratio found in such a kind of galaxy. Comparison with other Local Group dwarf spheroidals, Carina

    Fiorentino, G. et al.

    Fecha de publicación:

    11
    2012
    Número de citas
    21
  • On the Connection Between Solar Activity and Low-Latitude Aurorae in the Period 1715 - 1860

    Observations of aurorae borealis at low latitudes are very rare and are clearly associated with strong geomagnetic storms. Morphologically, they are characterized by a diffuse red colour with no rapid motions. The main aim of this paper is to analyse two hitherto ignored aurorae that were observed at two low-latitude sites, Tenerife (28°N 18°W) and

    Vázquez, M. et al.

    Fecha de publicación:

    11
    2006
    Número de citas
    17
  • On the dust content of galaxy clusters

    Context. Most of the contribution to dust emission in clusters of galaxies comes from late-type galaxies. However, several ejection processes of material from these galaxies could introduce dust in the intracluster media. Even a relatively low abundance of this dust could act as an efficient cooling agent and have a relevant role in the evolution

    Gutiérrez, C. M. et al.

    Fecha de publicación:

    11
    2014
    Número de citas
    27
  • On the effect of discrete numbers of stars in chemical evolution models

    We examine the impact of discrete numbers of stars in stellar populations on the results of Chemical Evolution Models. We explore the resulting dispersion in the true yields and their possible relation with the dispersion in observational data based on a Simple Closed-Box model. In this framework we find that the dispersion is larger for the less

    Cerviño, M. et al.

    Fecha de publicación:

    11
    2002
    Número de citas
    10
  • On the evolution of ejecta fragments in compact supernova remnants.

    The authors examine the evolution of inhomogeneities (fragments) of supernova ejecta in compact supernova remnants by means of hydrodynamical modelling and simplified analytical calculations. Under the influence of intense post-shock cooling the fragments become strongly compressed as they traverse the hot shocked region between the reverse and

    Miller, W. et al.

    Fecha de publicación:

    11
    1996
    Número de citas
    18