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

  • Narrow-band imaging - hit or miss?
    A reminder of the various factors that affect the central wavelength and bandpass of interference filters.
    King, D. et al.

    Fecha de publicación:

    6
    1994
    Número de citas
    2
  • Is GS:2000+25 an Eclipsing Black-Hole Binary
    We present an alternative interpretation of the quiescent optical light curve of GS2000 +25 published by Chevalier & Ilovaisky, and show that the modulation can be explained by a single periodicity. Using a method that is independent of the characteristics of the modulation of the light curve, we obtain an alternative value for the orbital period
    Shahbaz, T. et al.

    Fecha de publicación:

    6
    1994
    Número de citas
    12
  • IRAS 17423-1755: A BQ() star with a variable velocity outflow
    Infrared Astronomy Satellite (IRAS) 17423-1755 has been identified as a BQ() star. Its more remarkable observed features are large radial velocities, huge line widths and double-peaked profiles arising from its knots, and a high-velocity jet. Ejection velocity can account for the observational properties detected.
    Riera, A. et al.

    Fecha de publicación:

    6
    1994
    Número de citas
    1
  • Investigating the Kinematics of the Faint Giant Haloes of Planetary Nebulae
    Not Available
    Cuesta, L. et al.

    Fecha de publicación:

    6
    1994
    Número de citas
    0
  • Interstellar Na I absorption towards stars in the region of the IRAS Vela Shell.
    Not Available
    Srinivasan Sahu, M. et al.

    Fecha de publicación:

    6
    1994
    Número de citas
    4
  • Gravitational Radiation and Steady-State Distribution of Binary Orbits - Application to High-Mass Binary Pulsars
    By assuming the existence of a quasi-steady state of binary orbits of collapsed objects, a simple theory, relating the initial input distribution of semimajor axis and eccentricity to the steady-state distribution of these parameters, is formulated under the working hypothesis that the mechanism of variation of the above parameters is the emission
    Buitrago, J. et al.

    Fecha de publicación:

    6
    1994
    Número de citas
    7