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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  • Particle Accelerators in the Hot Spots of Radio Galaxy 3C 445, Imaged with the VLT
    Hot spots (HSs) are regions of enhanced radio emission produced by supersonic jets at the tip of the radio lobes of powerful radio sources. Obtained with the Very Large Telescope (VLT), images of the HSs in the radio galaxy 3C 445 show bright knots embedded in diffuse optical emission distributed along the post-shock region created by the impact of
    Prieto, M. A. et al.

    Fecha de publicación:

    10
    2002
    Número de citas
    36
  • A dynamical study of the circumstellar gas in UX Orionis
    We present the results of a high spectral resolution (lambda / Delta lambda = 49 000) study of the circumstellar (CS) gas around the intermediate mass, pre-main sequence star UX Ori. The results are based on a set of 10 échelle spectra covering the spectral range 3800-5900 Å, monitoring the star on time scales of months, days and hours. A large
    Mora, A. et al.

    Fecha de publicación:

    10
    2002
    Número de citas
    25
  • Detection of terrestrial planets and moons with the photometric transit method
    An overview is given over the photometric transit method for the detection of extraterrestrial planets. Discussed are: its basic principals, its derivable parameters, requirements for its implementation, and sources of confusion. Special emphasis is given space based experiments that may lead towards the detection of Earth-like planets. The
    Deeg, Hans J.

    Fecha de publicación:

    10
    2002
    Número de citas
    11
  • Thermal-magnetic relation of a sunspot as inferred from the inversion of 1.5 μm spectral data
    We present the thermal-magnetic relation in a simple, isolated sunspot deduced from the inversion of 1.56 μm spectropolarimetric data. Due to the high Zeeman sensitivity of the g = 3, Fe I 1.5648 μm line, we can study this relationship in the entire sunspot. An inversion technique based on response functions is used to derive various parameters
    Mathew, S. K. et al.

    Fecha de publicación:

    10
    2002
    Número de citas
    0
  • Thermal Dust Imaging of Massive Star-Forming Regions: W3 Main and W3 (OH)
    We present the preliminary results of mid-infrared images at 8.7, 9.7 and 12.5 micron of the complex massive star formation regions W3 Main and W 3(OH).
    Persi, P. et al.

    Fecha de publicación:

    10
    2002
    Número de citas
    0
  • Globular cluster formation from gravitational tidal effects of merging and interacting galaxies
    We investigate the spatial, kinematic and chemical properties of globular cluster systems formed in merging and interacting galaxies using N-body-smoothed particle hydrodynamics (SPH) simulations. Although we cannot resolve individual clusters in our simulation, we assume that they form in collapsing molecular clouds when the local external gas
    Bekki, K. et al.

    Fecha de publicación:

    10
    2002
    Número de citas
    86