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

  • Predictions of Ultraviolet Polarization and the Constraints Imposed on Dust Parameters
    Not Available
    Balcells, M. et al.

    Fecha de publicación:

    9
    1985
    Número de citas
    0
  • Photographic catalog of selected planetary size comparisons
    This publication utilizes photographs taken by NASA spacecraft, and cartographic products based on these photos, to illustrate size comparisons of the planets and moons of the solar system. It depicts both global views and prominent geographical features at the same scale, allowing size relationships to be studied visually.
    Meszaros, S. P.

    Fecha de publicación:

    9
    1985
    Número de citas
    0
  • Chromospheric modelling in late-type dwarfs. II - CES observations of active and quiescent stars
    The characteristics of the chromospheres of late-type dwarf stars were studied using the CoudeEchelle Spectrograph (CES) at ESO and the IUE. The study focused on the h and k Mg II lines of F and G dwarfs. The stability of the IUE spectra permitted calculations of averaged absorption features and the subtraction of the Mg II lines to leave intrinsic
    Foing, B. H. et al.

    Fecha de publicación:

    9
    1985
    Número de citas
    2
  • LETTERS AND COMMENTS: About a heuristic solution to the binding energy of the hydrogen atom
    Not Available
    Buitrago, J.

    Fecha de publicación:

    7
    1985
    Número de citas
    0
  • Dynamics of the dust material surrounding VEGA
    The spectrum corresponding to the emission of radiation from a dust distribution dominated by the dynamical action of the Poynting Robertson Effect is discussed and a model is applied to the dust surrounding Vega. It is found that a dust cloud extending from 41 to 177 AU match the 25, 60 and 100 micron measurements from IRAS. The 193 micron data
    Buitrago, J. et al.

    Fecha de publicación:

    7
    1985
    Número de citas
    19