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
    VIRGO: The solar monitor experiment on SOHO
    The VIRGO Experiment (Variability of solar IRradiance and Gravity Oscillations) contains two types of active cavity radiometers for monitoring of the solar constant, two three-channel Sun photometers 335, 500, and 865 nm, and a low resolution imager (LOI) with 12 pixels. The main scientific objective is probing the solar interior by helioseismology
    Froehlich, C. et al.

    Advertised on:

    12
    1988
    Bibcode
    1988ESASP.286..371F
    Citations
    2
  • Non-refereed
    The search for radial velocity variations in rapidly oscillating AP stars using the Fabry-Perot Interferometric Stellar Oscillation Spectrometer (FP-ISOS)
    Radial velocity measurements were taken of a group of Ap stars using an improved FP-ISOS. Observations were made using the 1.5m TCS on Tenerife in May 1987 and December 1987. The already known rapidly oscillating Ap stars 33 Lib and HR1217 were observed in order to search for radial velocity variations corresponding to the photometric periods found
    Leeper, M. et al.

    Advertised on:

    12
    1988
    Bibcode
    1988ESASP.286..587L
    Citations
    1
  • Non-refereed
    The GONG site survey.
    The Global Oscillation Network Group (GONG) project is planning to place six observing stations around the world to observe the solar oscillations as continuously as possible. This paper describes the procedures that are being used to select the six sites. The latest results of measurements of cloud cover obtained by networks of 6 (out of 10)
    Hill, F. et al.

    Advertised on:

    12
    1988
    Bibcode
    1988ESASP.286..209H
    Citations
    15
  • Refereed
    The chemical composition gradient across M 33
    The abundance gradient in M 33 is studied on the basis of IPCS and CCD data on emission lines in selected H II regions, using O II, O III, S II, and S III in the wavelength range 3700-9600 A to refine the oxygen abundances in the inner parts as well as to study the behavior of S/O. Spatially resolved observations in each H II region permit the
    Vilchez, J. M. et al.

    Advertised on:

    12
    1988
    Bibcode
    1988MNRAS.235..633V
    Citations
    283