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
    Near infrared morphology of M32.
    The authors present near infrared photometric observations in filters J and K of M32. Isophotal maps with an angular resolution of 93 pc are presented, radial J, K averaged profiles are derived and the characteristic surface brightness and effective radius are obtained.
    Cepa, J. et al.

    Advertised on:

    0
    1987
    Bibcode
    1987PAICz..69..335C
    Citations
    0
  • Non-refereed
    Near infrared morphology of M 32
    Near infrared photometric observations in filters J and K of M 32 are presented. Isophotal maps with an angular resolution of 93 pc are presented, radial J, K averaged profiles are derived, and the characteristic surface brightness and effective radius are obtained. The isophotal maps show a major axis angular displacement of 25 deg with respect to
    Cepa, J. et al.

    Advertised on:

    0
    1987
    Bibcode
    1987eram....4..335C
    Citations
    0
  • Non-refereed
    Intensity profiles in fluxtubes.
    Spectroscopic analysis of the light coming from an atmosphere is a powerful tool for revealing its properties. The problem when using conventional spectroscopy for solar fluxtubes is their unresolved character: magnetic and non-magnetic regions of a plage have to be observed as a whole. With the aim of obtaining the true intensity spectrum of an
    Sánchez Almeida, J. et al.

    Advertised on:

    0
    1987
    Bibcode
    1987PAICz..66..261S
    Citations
    0
  • Non-refereed
    Intensity profiles in fluxtubes
    A method is presented for reconstructing the intensity profile, I, formed in the magnetic elements which have diameters smaller than the best presently achievable spatial resolution. It follows the same line as in Solanki and Stenflo (1984). As a starting point I and V of the facula and the I observed in the quiet sun are used. The filling factor
    Sanches Almeida, J. et al.

    Advertised on:

    0
    1987
    Bibcode
    1987eram....1..261S
    Citations
    0