Publications

This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..

It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/

  • The Shape of the Luminosity Profiles of Bulges of Spiral Galaxies
    Using a 2D generalization of Kent's model-independent decomposition method, we extract the K-band light profiles of the bulges of a sample of field galaxies with morphological types ranging from S0 to Sbc. We then examine the shape of the bulge profiles, by means of fitting a seeing-convolved power law of the form μ(r) is proportional to r^1/n^
    Andredakis, Y. C. et al.

    Advertised on:

    8
    1995
    Citations
    330
  • The orbital period of CY UMa
    We present intermediate resolution spectroscopy of the dwarf nova CY UMa in quiescence. From the radial velocities of the Hα emission, we derive an orbital period of 0.067 95+/-8x10^-5 d, which disagrees with previous photometric estimates. We also constrain the system parameters. The core of the Hα emission seems to be dominated by a component
    Martinez-Pais, I. G. et al.

    Advertised on:

    8
    1995
    Citations
    7
  • The Hα environment of T Tauri resolved by speckle interferometry.
    T Tauri, the prototype of a class of low-mass pre-main sequence stars, was observed with the 3.6m Canada-France-Hawaii telescope (CFHT) and the CP40 photon-counting camera in November 1989. The data have been analysed using techniques of Speckle Interferometry to obtain diffraction-limited information on the spatial extent of T Tauri in narrow
    Bonneau, D. et al.

    Advertised on:

    8
    1995
    Citations
    8
  • The Extinction by Dust in the Outer Parts of Spiral Galaxies
    To investigate the distribution of dust in Sb and Sc galaxies we have analyzed near-infrared and optical surface photometry for an unbiased sample of 37 galaxies. Since light in the K-band is very little affected by extinction by dust, the B - K colour is a good indicator of the amount of extinction, and using the colour-inclination relation we can
    Peletier, R. F. et al.

    Advertised on:

    8
    1995
    Citations
    62
  • The chemical enrichment by massive stars in Wolf-Rayet galaxies.
    We present stellar population models for starbursts in a sample of eleven Wolf-Rayet galaxies. Taking into account the observational data available, we try to reconstruct the number of Wolf-Rayet stars observed and estimate the number of type II supernovae that have exploded in the ionizing cluster. Using the stellar yields of the most recent
    Esteban, C. et al.

    Advertised on:

    8
    1995
    Citations
    44
  • Sunspot activity curves and intermittent chaotic behavior.
    The authors analyze the statistical properties of observed sunspot numbers. Near the Maunder minimum, the dynamics of successive sunspot maxima is low-dimensional and has properties similar to the intermittent logistic map. The long-term statistics is well described by an intermittent random injection model with Poissonian injection statistics
    Gurbuz, G. et al.

    Advertised on:

    8
    1995
    Citations
    2