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..

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  • Observational studies of Cepheid amplitudes. I. Period-amplitude relationships for Galactic Cepheids and interrelation of amplitudes
    Context: The dependence of amplitude on the pulsation period differs from other Cepheid-related relationships. Aims: We attempt to revise the period-amplitude (P-A) relationship of Galactic Cepheids based on multi-colour photometric and radial velocity data. Reliable P-A graphs for Galactic Cepheids constructed for the U, B, V, R_C, and IC
    Klagyivik, P. et al.

    Fecha de publicación:

    9
    2009
    Número de citas
    69
  • Multiwavelength Observations Of Comet 67p/Churyumov-Gerasimenko During Its Approach To Perihelion
    Comet 67P, the target of Rosetta mission, was observed in the visible and near-IR spectral regions during its perihelion approach. The observations were performed in four epochs, at heliocentric distances varying from about 3 to 1.4 AU, i. e. in the same range of the Rosetta mission. The aims of the observations were the study of the dust coma and
    Tozzi, Gian-Paolo et al.

    Fecha de publicación:

    9
    2009
    Número de citas
    0
  • Multiline Zeeman signatures through line addition
    Context: To obtain a significant Zeeman signature in the polarised spectra of a magnetic star, we usually “add” the contributions of numerous spectral lines; the ultimate goal is to recover the spectropolarimetric prints of the magnetic field in these line additions. Aims: Here we want to clarify the meaning of these techniques of line addition; in
    Semel, M. et al.

    Fecha de publicación:

    9
    2009
    Número de citas
    31
  • Multi-wavelength observations of the GRB 080319B afterglow and the modeling constraints
    Context: We present observations of the GRB 080319B afterglow at optical, mm, and radio frequencies between a few hours and 67 days after the burst. Aims: We attempt to understand the nature of this extraordinarily bright explosion based on the observed properties and its comparison with afterglow models. Methods: Our observations and other
    Pandey, S. B. et al.

    Fecha de publicación:

    9
    2009
    Número de citas
    25
  • Morphology and evolution of umbral dots and their substructures
    Context: Substructures - dark lanes and tails - of umbral dots (UDs) were predicted by numerical simulations of magnetoconvection and have been detected later in some observations. Aims: To provide constraints for realistic theoretical models of sunspot umbrae, we describe the observed properties and evolutionary characteristics of UDs (including
    Sobotka, M. et al.

    Fecha de publicación:

    9
    2009
    Número de citas
    37
  • Monitoring of geological activity on astronomical sites of the Canary Islands, Hawaii, and Chile
    Future large and extremely large ground-based telescopes will demand stable geological settings.Remote sensing could be an unvaluable tool to analyse the impact of geological activity at selected astronomical sites, namely the observatories of El Teide (Tenerife, Canary Islands), Roque de los Muchachos (La Palma, Canary Islands), Mauna Kea (Hawaii)
    Eff-Darwich, Antonio et al.

    Fecha de publicación:

    9
    2009
    Número de citas
    0