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
    Contribution of Low-l P Modes to the Solar Equatorial Rotation Profile
    The solar equatorial velocity profile is known down to the base of the convection zone with high precision (
    Rabello Soares, M. C. et al.

    Advertised on:

    5
    1997
    Bibcode
    1997ApJ...480..840R
    Citations
    5
  • Refereed
    Variable central stars of young planetary nebulae. I. Photometric multisite observations of IC 418.
    We report the results of a photometric multisite campaign devoted to HD 35914, the variable central star of the Planetary Nebula IC 418. From the analysis of 120 hours of data acquired with a variety of techniques, we find that HD 35914 exhibits two distinct kinds of variability: irregular light modulation with a time scale of days, as well as
    Handler, G. et al.

    Advertised on:

    4
    1997
    Bibcode
    1997A&A...320..125H
    Citations
    22
  • Refereed
    Time Delay of QSO 0957+561 and Cosmological Implications
    We obtain the time delay between the arrival time of the A and B images of the QSO 0957+561. The results of applying two different methods (the discrete cross-correlation function and the dispersion estimation technique) to the observed light curves of the A and B images are presented. The adopted value (time delay) is of Delta tau BA = 424 +/- 3
    Oscoz, Alejandro et al.

    Advertised on:

    4
    1997
    Bibcode
    1997ApJ...479L..89O
    Citations
    37
  • Refereed
    The black hole transient Nova Scorpii 1994 (=GRO J1655-40): orbital ephemeris and optical light curve
    We have measured the brightness of the optical counterpart of the black hole X-ray binary Nova Sco 1994 (GRO J1655-40) during 40 nights between 1995 May 3 and July 27. From our observations and data from the literature we refine the orbital period to be 2.620 40+/-0.000 98 d. We model the R-band light curve as primarily arising from an X-ray heated
    van der Hooft, F. et al.

    Advertised on:

    4
    1997
    Bibcode
    1997MNRAS.286L..43V
    Citations
    21