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

  • Classification and vsini of Vega-type and PMS stars (Mora+, 2001)
    File table1.dat contains the log of the spectroscopic observations of the stars in the EXPORT sample taken with the Isaac Newton Telescope during the 1998 International Time Campaigns at the Canary Islands' Observatories. File table2.dat contains the log of the spectroscopic observations of the stars in the EXPORT sample taken with the William
    Mora, A. et al.

    Fecha de publicación:

    9
    2001
    Número de citas
    0
  • Climatology at the Roque de LOS Muchachos Observatory
    The Roque de los Muchachos Observatory (ORM) at La Palma (Canary Islands) is one of the two top pre-selected sites for hosting the future European Extremely Large Telescope (E-ELT), the other ones are Ventarrones (Chile), Macon (Argentine) and Aklim (Maroc). Meteorological and seeing conditions are crucial both for the site selection and for
    Varela, Antonia M. et al.

    Fecha de publicación:

    9
    2009
    Número de citas
    2
  • Cluster Emission of $^8$Be in the $^{28}$Si+$^{12}$C Fusion Reaction at Low Temperature
    Inclusive as well as exclusive energy spectra of the light charged particles emitted in the $^{28}$Si ($E_{lab}$=112.6 MeV) + $^{12}$C reaction has been measured using the {f ICARE} multidetector array. The data have been analysed by statistical-model calculations using a spin-dependent level density parametrization. The results suggest
    Rousseau, M. et al.

    Fecha de publicación:

    9
    1999
    Número de citas
    0
  • CN and CH line strengths in 12 globulars (Pancino+, 2010)
    In this first paper, we measured the strength of the CN and CH band indices, which correlate with the N and C abundances, and we investigated the anti-correlation and bimodality of these indices. We compared rCN, the ratio of stars belonging to the CN-strong and weak groups, with 15 different cluster parameters. (1 data file).
    Pancino, E. et al.

    Fecha de publicación:

    9
    2010
    Número de citas
    0
  • CO (3-2) Observations of Early-Type Galaxies with the Heinrich Hertz Telescope
    We present Heinrich Hertz Telescope CO (3-2) observations of a sample of 10 early-type galaxies detected both in far-infrared (IRAS) and in CO (1-0). Six of the objects (i.e., 60% of the sample) were detected in the CO (3-2) transition. Comparison of the beam-matched CO (3-2)/CO (1-0) and CO (2-1)/CO (1-0) intensity ratios with simple large
    Vila-Vilaró, B. et al.

    Fecha de publicación:

    9
    2003
    Número de citas
    14
  • CO emission from candidate photo-dissociation regions in M 81
    Context: .At least a fraction of the atomic hydrogen in spiral galaxies is suspected to be the result of molecular hydrogen which has been dissociated by radiation from massive stars. Aims: .In this paper, we extend our earlier set of data from a small region of the Western spiral arm of M 81 with CO observations in order to study the interplay
    Knapen, J. H. et al.

    Fecha de publicación:

    9
    2006
    Número de citas
    7