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/

  • Refereed
    Dust in the nuclei of the Seyfert galaxies Markarian 231 and NGC 4151
    Observations carried out with a 8-13 micron grating-spectrometer of Mrk 231 and NGC 4151 are reported. The Mrk 231 data can be fitted to various thermal dust emission models or a single power law, with dust extinction. In all the model fits, except for that of graphite and silicon carbide grain emission, a component of silicate absorption of
    Jones, B. et al.

    Advertised on:

    9
    1984
    Bibcode
    1984PASP...96..692J
    Citations
    6
  • Refereed
    A survey of faint, near-infrared sources towards the centre of the Galaxy
    The authors present the results of a survey made at 1.65 μm (H) and 2.2 μm (K) in 15 small areas on the galactic equator between l = 0° and l = 10°. 775 distinct objects were counted in a total area of 0.17 deg2 to limiting magnitudes H = 10.5 and K = 9.5 (equivalent to detecting M giants at 6 - 7 kpc). Source confusion was the limiting factor in
    Jones, A. W. et al.

    Advertised on:

    9
    1984
    Bibcode
    1984A&A...138..297J
    Citations
    7
  • Non-refereed
    Nova Vulpeculae 1984
    IAUC 3977 available at Central Bureau for Astronomical Telegrams. IAUC 3977 available at Central Bureau for Astronomical Telegrams.
    Maley, P. et al.

    Advertised on:

    8
    1984
    Bibcode
    1984IAUC.3977....3M
    Citations
    0
  • Non-refereed
    Use of high resolution IUE spectra of MG 2 in cool stars to probe the local interstellar medium
    It is shown that, given suitable radial velocity values for the stars and the local interstellar medium (LISM) interstellar absorption can be distinguished from chromospheric self absorption within the MgII emissions from late type stars. Beta Hyi (G2IV) offers a clear example. Zeta Tuc (G2V) and delta Pav (G8V) which are very close to beta Hyi
    Molaro, P. et al.

    Advertised on:

    7
    1984
    Bibcode
    1984ESASP.218..139M
    Citations
    3