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/

  • STEPHI-92 - Bn-Cancri and Bu-Cancri - Two Delta-Scuties in the Praesepe Cluster
    Not Available
    Belmonte, J. A. et al.

    Advertised on:

    1
    1993
    Citations
    11
  • Starburst ages in HII galaxies
    The age of the starbursts of a few H2 galaxies is derived from optical photometry and compared with previous results from radio continuum spectra. H2 galaxies are gas rich and characterized by the dominance of giant H2 regions, blue stellar colors, high surface brightness, and narrow emission lines. The presently observed high abundances of bright
    Deeg, Hans-Joerg

    Advertised on:

    1
    1993
    Citations
    1
  • Spectroscopy and shock modelling of the unusual bipolar outflow NGC 6905
    We present high and low resolution multi-slit spectroscopy, together with V, forbidden O III, and H-alpha narrow band imaging of the unusual bipolar outflow source NGC 6905. As a consequence, we are able to investigate the excitation structure of the source, the properties of the central star, and the projected kinematic structure of the outflow
    Cuesta, L. et al.

    Advertised on:

    1
    1993
    Citations
    26
  • Searching for emission-line galaxies: The UCM survey
    We are carrying out a long-term project with the main purposes of finding and analyzing low metallicity galaxies. A very small number of very low metallicity galaxies is known up to now. However these ojbects are particularly interesting since they are excellent candidates to 'young galaxies' in evolutionary sense as POX186 (Kunth, Maurogordato &
    Gallego, J. et al.

    Advertised on:

    1
    1993
    Citations
    0
  • SAO 244567 - A post-AGB star which has turned into a planetary nebula within the last 40 years
    SAO 244567 (Hen 1357 = CPD -59 deg 6926 = IRAS 17119-5926) is an IRAS source with far infrared colors and flux distribution similar to those of planetary nebulae. The IUE ultraviolet spectra obtained in July 1988 and April 1992 show nebular emission lines, and also the changes in the spectra suggest the formation of the planetary nebula and the
    Parthasarathy, M. et al.

    Advertised on:

    1
    1993
    Citations
    65