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

  • Long-slit echelle spectroscopy at the NTT.
    During our recent observing run at La Silla (April 26-28, 1996), we had the chance to experiment successfully a previously unexplored capability of the NTT: high-dispersion spectroscopy using the full slit length of EMMI.
    Corradi, R. L. M. et al.

    Fecha de publicación:

    9
    1996
    Número de citas
    8
  • IZw18 has a Dynamically Associated Companion Galaxy
    We present kinematical evidence that the irregular galaxy located 26'' northwest of IZw18 -the most metal-poor blue-compact-dwarf (BCD) galaxy known- is a dynamically associated companion system. Longslit CCD spectra were obtained in 1996 February using the 4.2m WHT+ISIS at La Palma, with the slit placed across the NW HII region of IZw18 and
    Dufour, R. J. et al.

    Fecha de publicación:

    9
    1996
    Número de citas
    0
  • Irregular variables of type Lb. New JHKL'M-photometry for 160 stars.
    This paper presents new near infrared observations of 160 Irregular variables of type Lb in the JHKL'M filter bands. These measurements are supplemented by data for additional 56 stars taken from the literature. In total 220 datasets are available because of some multiple observations. From our sample, 216 stars have near infrared (NIR) photometry
    Kerschbaum, F. et al.

    Fecha de publicación:

    9
    1996
    Número de citas
    26
  • Iron abundance and dust in galactic H II regions.
    The [Fe II] and [Fe III] emission of seven galactic H II regions is studied with the aim of comparing their gaseous Fe abundance. The [Fe II] line intensity ratios are found to behave in a manner that suggests fluorescence effects. In addition, the uncertainty in the physical conditions and the ionization stratification of the layers where [Fe II]
    Rodriguez, M.

    Fecha de publicación:

    9
    1996
    Número de citas
    27
  • Detection of Habitable-Sized Planets: A Progress Report
    Planets forming around close binary systems should form in the binary orbital plane (varying precession periods of protoplanetary material should provide strong collisional damping; Schneider and Doyle 1995). Planets around eclipsing binaries may then be expected to have formed in the binary orbital plane and thus to be detected by their transits
    Doyle, L. R. et al.

    Fecha de publicación:

    9
    1996
    Número de citas
    0
  • Constraints on the use of Be I lines for deriving beryllium abundances in late-type dwarf stars.
    Beryllium is a key element for constraining mixing processes taking place in the interiors of late-type dwarfs, and this paper investigates the use of neutral beryllium lines to obtain reliable abundances. The best candidate, among other Bei features, is the ^9^Bei λ2348.609A resonance line. Its spectral location, well below the Earth's UV
    Garcia Lopez, R. J.

    Fecha de publicación:

    9
    1996
    Número de citas
    5