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
    Narrow-band imaging - hit or miss?
    A reminder of the various factors that affect the central wavelength and bandpass of interference filters.
    King, D. et al.

    Advertised on:

    6
    1994
    Bibcode
    1994IEEES...2...20K
    Citations
    2
  • Refereed
    Is GS:2000+25 an Eclipsing Black-Hole Binary
    We present an alternative interpretation of the quiescent optical light curve of GS2000 +25 published by Chevalier & Ilovaisky, and show that the modulation can be explained by a single periodicity. Using a method that is independent of the characteristics of the modulation of the light curve, we obtain an alternative value for the orbital period
    Shahbaz, T. et al.

    Advertised on:

    6
    1994
    Bibcode
    1994MNRAS.268..763S
    Citations
    12
  • Refereed
    IRAS 17423-1755: A BQ() star with a variable velocity outflow
    Infrared Astronomy Satellite (IRAS) 17423-1755 has been identified as a BQ() star. Its more remarkable observed features are large radial velocities, huge line widths and double-peaked profiles arising from its knots, and a high-velocity jet. Ejection velocity can account for the observational properties detected.
    Riera, A. et al.

    Advertised on:

    6
    1994
    Bibcode
    1994Ap&SS.216...43R
    Citations
    1
  • Non-refereed
    Interstellar Na I absorption towards stars in the region of the IRAS Vela Shell.
    Not Available
    Srinivasan Sahu, M. et al.

    Advertised on:

    6
    1994
    Bibcode
    1994Msngr..76...48S
    Citations
    4
  • Refereed
    Gravitational Radiation and Steady-State Distribution of Binary Orbits - Application to High-Mass Binary Pulsars
    By assuming the existence of a quasi-steady state of binary orbits of collapsed objects, a simple theory, relating the initial input distribution of semimajor axis and eccentricity to the steady-state distribution of these parameters, is formulated under the working hypothesis that the mechanism of variation of the above parameters is the emission
    Buitrago, J. et al.

    Advertised on:

    6
    1994
    Bibcode
    1994MNRAS.268..841B
    Citations
    7