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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  • Evolution of active galactic nuclei broad-line region clouds: low- and high-ionization lines
    The formation of quasar broad-line region (BLR) clouds via thermal instability in the presence of Alfvén heating has been discussed by Gonçalves, Jatenco-Pereira & Opher. In particular, these studies showed the relevance of Alfvén heating in establishing the stability of BLR clouds in the intercloud medium. The present paper shows the results of
    Gonçalves, D. R. et al.

    Fecha de publicación:

    12
    2001
    Número de citas
    3
  • Erratum: ``H I in the Shell Elliptical Galaxy NGC 3656'' [Astron. J. 122, 1758 (2001)]
    As the result of an editorial oversight, the following two works were misattributed in the references:Schweizer, F. 1998, in Galaxies: Interactions and Induced Star Formation, ed. D. Friedli, L. Martinet, & D. Pfenniger (Berlin: Springer), 105Sparke, L. S. 1996, ApJ, 473, 810The publisher regrets the error.
    Balcells, Marc et al.

    Fecha de publicación:

    12
    2001
    Número de citas
    1
  • Diffuse Emission in the Nucleus of M31
    We will present analysis of the diffuse emission from the nucleus of M31 using a 40 ks Chandra ACIS-S observation. The observation was taken by Chandra on 5 October, 2001. This is a continuation of our work performed on a 5 ks observation with the Chandra ACIS-I detector, presented as a poster paper at the 2001 ASP conference. With this observation
    Dosaj, A. et al.

    Fecha de publicación:

    12
    2001
    Número de citas
    1
  • Chandra observations of the radio jets in a sample of quasars
    We present the results from an X-ray and optical survey of a sample of radio jets in AGN with Chandra and HST. We focus on the first six sources observed at X-rays, in four of which a bright X-ray jet was detected for the first time. In three out of four cases optical emission from the jet is also detected in the HST images. We compare the X-ray
    Sambruna, R. M. et al.

    Fecha de publicación:

    12
    2001
    Número de citas
    0
  • Chandra Multiwavelength Plane Survey (ChaMPlane): Photometry Results from the First Two Years
    We present the photometric results of the Chandra Multiwavelength Plane Survey (ChaMPlane), which is a project to identify a large sample of serendipitous X-ray sources in the galactic plane, in order to determine the populations of accretion-powered binaries in the Galaxy. Deep Chandra field observations have sufficient sensitivity to reach
    Zhao, P. et al.

    Fecha de publicación:

    12
    2001
    Número de citas
    0
  • Chandra Multiwavelength Plane (ChaMPlane) Survey: Initial X-ray Results
    The ChaMPlane survey of the galactic plane ( ~100 ACIS fields over 5 years, selected for exposure at least ~20ksec, galactic latitude below ~10deg, and minimum column density NH), will provide the largest sample of faint galactic x-ray sources. The arcsec positions for most of these will allow unambiguous optical identifications from our NOAO Long
    Grindlay, J. et al.

    Fecha de publicación:

    12
    2001
    Número de citas
    0