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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  • EXPORT: Optical photometry and polarimetry of Vega-type and pre-main sequence stars
    This paper presents optical UBVRI broadband photo-polarimetry of the EXPORT sample obtained at the 2.5 m Nordic Optical Telescope. The database consists of multi-epoch photo-polarimetry of 68 pre-main-sequence and main-sequence stars. An investigation of the polarization variability indicates that 22 objects are variable at the 3sigma level in our
    Oudmaijer, R. D. et al.

    Fecha de publicación:

    11
    2001
    Número de citas
    106
  • Extended coronal emission lines in active galactic nuclei
    VLT and NTT spectra are used to examine the nuclear and extended coronal line emission in a sample of well-known Seyfert 1 and 2 galaxies. The excellent spatial resolution obtained with VLT allowed us to map [Si VI] 1.963μm and [Si VII] 2.48μm on scales of up to 20 pc. Coronal line emission, extended to distances of ˜102 pc, is detected in some of
    Rodríguez-Ardila, Alberto et al.

    Fecha de publicación:

    11
    2004
    Número de citas
    4
  • Extended line emission in AGN: Looking at the central engine
    The regions of high excitation gas detected around various Active Galactic Nuclei (AGN) are examined. The radiation emitted by the nucleus may be responsible for the high ionization of the line emitting gas. Evidence that the radiation field is anisotropic and collimated in a direction close to the cone axis is found. The possibility that a
    Acosta Pulido, J. et al.

    Fecha de publicación:

    11
    1989
    Número de citas
    0
  • Extended line emission in AGN: looking at the central engine.
    Regions of high excitation gas were detected around various active galactic nuclei. Their shape resembles a cone whose axis is oriented close to the radio axis. The radiation emitted by the nucleus may be responsible for the high ionization of the line emitting gas. Moreover there is evidence that the radiation field should be anisotropic and
    Pulido, J. A. et al.

    Fecha de publicación:

    11
    1989
    Número de citas
    0
  • Extended warm gas in the ULIRG Mrk273: Galactic outflows and tidal debris
    We present new HST/ACS medium- and narrow-band images and optical Isaac Newton Telescope long-slit spectra of the merging system Mrk273. The HST observations sample the [OIII]λλ4959,5007 emission from the galaxy and the nearby continuum. These data were taken as a part of a larger study of ultraluminous infrared galaxies (ULIRGs) with the aim of
    Rodríguez Zaurín, J. et al.

    Fecha de publicación:

    11
    2014
    Número de citas
    13
  • Extinction over the Canarian observatories: the limited influence of Saharan dust
    We present a study of the atmospheric extinction over the observatories of the Canary Islands, based mainly on photometric measurements of the V-band extinction coefficient obtained during /2850 nights at the Carlsberg Automatic Meridian Circle at the Roque de los Muchachos Observatory (La Palma), and complemented with visible and infrared data
    Guerrero, M. A. et al.

    Fecha de publicación:

    11
    1998
    Número de citas
    14