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/

  • Looking through the dust - the edge-on galaxy NGC 7814 in the near-infrared.
    Not Available
    Peletier, R. F. et al.

    Advertised on:

    12
    1992
    Citations
    3
  • Geochemistry of HASP, VLT, and other glasses from double drive tube 79001/2
    The Apollo 17 double drive tube 79001/2 (station 9, Van Serg Crater) is distinctive because of its extreme maturity, abundance, and variety of glass clasts. It contains mare glasses of both high Ti and very low Ti (VLT) compositions, and highland glasses of all compositions common in lunar regolith samples: highland basalt (feldspathic; Al2O3
    Lindstrom, D. J. et al.

    Advertised on:

    12
    1992
    Citations
    0
  • Are QSOs more highly polarized than QSSs?
    We have observed a sample of "ordinary" quasars, selected only on the grounds of their relative brightness in the visible, with the Turku Photopolarimeter on the 2.56m Nordic Optical Telescope, on La Palma, Canary Islands. The instrument permits us to obtain simultaneous UBVRI photometry and polarimetry of objects down to 16th magnitude, with the
    Takalo, L. O. et al.

    Advertised on:

    12
    1992
    Citations
    0
  • A Radio-Optical Study of HII galaxies
    A detailed insight into the star formation history of a sample of HII galaxies has been obtained, based on radio continuum and optical broad band and narrow band observations. HII galaxies are dwarf galaxies whose optical spectrum resembles that of HII regions, many of which are also known as Blue Compact Dwarf Galaxies. VLA observations at several
    Deeg, Hans-Jorg

    Advertised on:

    12
    1992
    Citations
    0
  • A Radio Continuum Search for Twelve Low Surface Brightness Dwarf Galaxies
    The radio properties of low surface brightness (LSB) dwarf galaxies are still largely unknown. To help remedying this situation we observed twelve LSB dwarfs with the VLA at lambda = 3.6 cm and lambda = 20 cm. All galaxies are included in the UGC catalog and have previously claimed radio continuum detections at either 21 cm (Altschuler et al. 1984
    Hoeppe, G. et al.

    Advertised on:

    12
    1992
    Citations
    0