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 ROSAT UK Medium Sensitivity Survey: optical identification and relation to X-ray spectral properties
    We present the first results on the optical identification of 89 sources with S(0.5-2 keV)>=1.7x10^-14 erg s^-1 cm^-2 detected in eight ROSAT Position Sensitive Proportional Counter (PSPC) observations targeted on the second Lockman hole region. Because of the low Galactic HI column density towards this field [N_HI~(6-12)x10^19 cm^-2] the X-ray
    Carballo, R. et al.

    Advertised on:

    12
    1995
    Citations
    39
  • The outflow structure of NGC 6537.
    We present high and low resolution spectroscopy and narrow-band imaging of the unusual bipolar outflow source NGC 6537. As a consequence, we are able for the first time to construct large scale velocity maps of this source; note the presence of strongly variable core outflow densities, rising to a peak value n_e_~1.7x10^4^cm^-3^; find evidence for
    Cuesta, L. et al.

    Advertised on:

    12
    1995
    Citations
    23
  • The Effect of Temperature Fluctuations on the Determination of the Carbon Abundances of Planetary Nebulae
    Not Available
    Peimbert, M. et al.

    Advertised on:

    12
    1995
    Citations
    3
  • The Central Region in M100: Observations and Modeling
    We present new high-resolution observations of the central region in the late-type spiral galaxy M100 (NGC 4321) supplemented by three-dimensional numerical modeling of stellar and gas dynamics, including star formation (SF). Near-infrared imaging has revealed a small bulge of 4" effective diameter; a 60" radial length stellar bar of moderate
    Knapen, J. H. et al.

    Advertised on:

    12
    1995
    Citations
    242
  • Stellar models for a wide range of initial chemical compositions until helium burning. II. From X=0.63 to X=0.80, for Z=0.01.
    Three new grids of stellar evolutionary models with Z=0.01 are presented for the following values of initial hydrogen content X_i_=0.80, 0.73 and 0.63. The latest set of radiative opacities with spin-orbit coupling provided by the Lawrence Livermore group are used. For the lower temperatures the results by Alexander were considered. The models were
    Gimenez, A. et al.

    Advertised on:

    12
    1995
    Citations
    43