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/

  • Non-refereed
    Radio to γ-ray observations of 3C 454.3:1993-1995
    Results from a multiwaveband study of the γ-ray-bright compact radio source 3C 454.3 are presented.
    Aller, M. F. et al.

    Advertised on:

    5
    1997
    Bibcode
    1997AIPC..410.1423A
    Citations
    7
  • Refereed
    Quantitative spectroscopic criteria for the classification of pre-main sequence low-mass stars.
    The discovery of hundreths of X-ray emitting stars possibly associated with pre-main sequence (PMS) low-mass stars far from molecular clouds, makes it necessary to adopt quantitative spectroscopic criteria for classifying them. T Tauri stars have young ages (
    Martin, E. L.

    Advertised on:

    5
    1997
    Bibcode
    1997A&A...321..492M
    Citations
    95
  • Non-refereed
    Old Populations and the Star Formation History of the Local Group Dwarf Irregular Galaxy NGC 6822
    A method for studying the full star formation history (SFH) of nearby galaxies,as a function of time, has been developped and implemented. For the first time, the full SFH of a nearby dwarf irregular galaxy (DIG) has been retrieved from the photometry of its resolved stars. NGC~6822 has been observed in $UBVRI$ at the 2.5m INT telescope, at the
    Gallart, C.

    Advertised on:

    5
    1997
    Bibcode
    1997PASP..109..629G
    Citations
    1
  • Non-refereed
    Old Populations and the Star Formation History of the Local Group Dwarf Irregular Galaxy NGC 6822
    A method for studying the star formation history (SFH) of nearby galaxies, as a function of time, has been developped and implemented. For the first time, the full SFH of a nearby dwarf irregular galaxy (DIG) has been retrieved from the photometry of its resolved stars. In the [(V-I),I] colour-magnitude diagram (CMD) of about 18000 stars in NGC
    Gallart, C. et al.

    Advertised on:

    5
    1997
    Bibcode
    1997AAS...190.3506G
    Citations
    0