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
    Observational patterns of lithium depletion in pre-main sequence stars
    Not Available
    Martín, E. L. et al.

    Fecha de publicación:

    1
    1993
    Bibcode
    1993ASPC...40..165M
    Número de citas
    3
  • Con árbitro
    Near-infrared photometry and spectrophotometry of two unusual novae
    We present near IR photometry and spectrophotometry of two unusual novae observed in 1991: Nova Herculis and Nova Scuti. Both are seen to have unusual spectral and light curve characteristics, the former due to the very formation of a dust cloud surrounding the nova and the second because of what is interpreted to be high interstellar reddening
    Kidger, M. R. et al.

    Fecha de publicación:

    1
    1993
    Bibcode
    1993A&A...267..111K
    Número de citas
    3
  • Sin árbitro
    Narrow band imaging and long slit spectroscopy of UGC 5101
    UGC 5101 (z = 0.04; D is approximately equal to 240 Mpc) is one of the so called Ultraluminous IRAS sources. Two important properties of the members of this group are their L(sub IR) is greater than or equal to 10(exp 12) solar luminosity, and their space density in the universe up to z is less than 0.1 is equal or even larger than the space
    Stanga, R. M. et al.

    Fecha de publicación:

    1
    1993
    Bibcode
    1993egte.conf..317S
    Número de citas
    0
  • Con árbitro
    Multiple frequencies of the δ Scuti variable HD213534
    By a large number of high-precision photoelectric photometry data obtained in three sites, making use of the method of Fourier Period Analysis, the multiple frequencies of HD213534 have been obtained. Five frequencies have been definitely detected. Through the discussion of the pulsation modes of the star, we tended to believe that it is a multiple
    Fu, Jian-Ning et al.

    Fecha de publicación:

    1
    1993
    Bibcode
    1993ChA&A..17...65F
    Número de citas
    0