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

  • Sin árbitro
    Light curve morphology of TT Ari in the recent state of apsidal superhump
    Not Available
    Piccioni, A. et al.

    Fecha de publicación:

    0
    2005
    Bibcode
    2005foap.conf..677P
    Número de citas
    0
  • Sin árbitro
    Interannual to decadal sea level change in south-western Europe from satellite altimetry and in-situ measurements
    Not Available
    Fenoglio-Marc, L. et al.

    Fecha de publicación:

    0
    2005
    Bibcode
    2005ggsm.conf..242F
    Número de citas
    0
  • Sin árbitro
    IMF variations in dwarf galaxies
    Dwarf galaxies tend to have a large spread in metal abundances and overall lower metallicites than large Spiral or Elliptical ones. Here we propose that if all stars are formed from an invariant canonical IMF within each star cluster which are distributed according to an embedded cluster mass function (ECMF), then the integrated stellar IMF over
    Weidner, C. et al.

    Fecha de publicación:

    0
    2005
    Bibcode
    2005nfcd.conf..130W
    Número de citas
    0
  • Sin árbitro
    High mass Star formation in the giant molecular cloud NGC 6334: an infrared view
    Sub-Arcsec images in the JHK_s, H_2 and Br_γ of three areas (I(N), F and NGC 6334 IV (MM3)) of the giant molecular cloud NGC 6334 are presented. The preliminary results indicate the presence of a deeply embedded young stellar cluster in the northermost part of the cloud (I(N)). We have identified the exciting source of the cometary UCHII NGC 6334 F
    Persi, P. et al.

    Fecha de publicación:

    0
    2005
    Bibcode
    2005IAUS..227..291P
    Número de citas
    8
  • Sin árbitro
    Heights of formation of Mn I spectral lines broadened by hyperfine structure
    This paper considers the influence of hyperfine broadening on heights of formation of some Mn I spectral lines in Solar spectrum. The comprehensive model atom of neutral manganese is constructed with 64 bound energy levels and continuum and 161 bound-bound transitions. Preliminary results of spectrum synthesis for this model and atmospheric models
    Vitas, N.

    Fecha de publicación:

    0
    2005
    Bibcode
    2005MSAIS...7..164V
    Número de citas
    4