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/

  • Deconstructing the Quiescent Black Hole V404 Cyg

    The black hole binary V404 Cyg has provided a primary test bed for models of accretion in quiescent black hole binaries because it is by far the brightest in the X-ray band. Most published work, however, has been based on non-simultaneous data spanning many years since its major outburst in 1989. We present the most complete spectral energy

    Hynes, Robert I. et al.

    Advertised on:

    9
    2006
    Citations
    0
  • Decreased Frequency of Strong Bars in S0 Galaxies: Evidence for Secular Evolution?

    Using data from the Near-Infrared S0 Survey of nearby, early-type galaxies, we examine the distribution of bar strengths in S0 galaxies as compared to S0/a and Sa galaxies, and as compared to previously published bar strength data for Ohio State University Bright Spiral Galaxy Survey spiral galaxies. Bar strengths based on the gravitational torque

    Buta, R. et al.

    Advertised on:

    9
    2010
    Citations
    45
  • Deep CCD photometry of stars in the globular cluster M3

    CCD photometry of faint stars in the globular cluster M3 is presented. The observations reach down to V equal to about 23 mag, with a sample of approximately 5000 stars. The resulting color magnitude diagram has a turn-off significantly redder than those obtained in previous studies. Age and distance are derived by fitting the observed mean line to

    Paez, E. et al.

    Advertised on:

    9
    1990
    Citations
    25
  • Deep echelle spectrophotometry of S 311, a Galactic HII region located outside the solar circle

    We present echelle spectrophotometry of the Galactic HII region S 311. The data have been taken with the Very Large Telescope Ultraviolet-Visual Echelle Spectrograph in the 3100-10400 Årange. We have measured the intensities of 263 emission lines; 178 are permitted lines of H0, D0 (deuterium), He0, C0, C+, N0, N+, O0, O+, S+, Si0, Si+, Ar0 and Fe0

    García-Rojas, J. et al.

    Advertised on:

    9
    2005
    Citations
    83
  • Deep Emission Line Images of the Extended Narrow Line Region: Mapping the Ionizing Cones in Seyfert Galaxies

    Not Available

    Wilson, A. S. et al.

    Advertised on:

    9
    1988
    Citations
    0
  • Deep SDSS optical spectroscopy of distant halo stars. III. Chemical analysis of extremely metal-poor stars

    Aims: We present the results of an analysis of 107 extremely metal-poor (EMP) stars with metallicities lower than [Fe/H] =- 3.0, identified in medium-resolution spectra in the Sloan Digital Sky Survey (SDSS). Our analysis provides estimates of the stellar effective temperatures and surface gravities, as well as iron, calcium, and magnesium

    Schneider, D. P. et al.

    Advertised on:

    9
    2016
    Citations
    8