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
    How does breakup influence near-barrier fusion of weakly bound light nuclei ?
    The influence on the fusion process of coupling to collective degrees of freedom has been explored. The significant enhancement of he fusion cross setion at sub-barrier energies was understood in terms of the dynamical processes arising from strong couplings to collective inelastic excitations of the target and projectile. However, in the case of
    Beck, C. et al.

    Advertised on:

    11
    2004
    Bibcode
    2004nucl.ex..11002B
    Citations
    10
  • Refereed
    How large are the bars in barred galaxies?
    I present a study of the sizes (semimajor axes) of bars in disc galaxies, combining a detailed R-band study of 65 S0-Sb galaxies with the B-band measurements of 70 Sb-Sd galaxies from Martin (1995). As has been noted before with smaller samples, bars in early-type (S0-Sb) galaxies are clearly larger than bars in late-type (Sc-Sd) galaxies; this is
    Erwin, Peter

    Advertised on:

    11
    2005
    Bibcode
    2005MNRAS.364..283E
    Citations
    198
  • Refereed
    How to determine the quality of solar granulation images: The optimal window method
    An optimal window for image analysis is determined by means of information theory. The size of the window is then used as a good estimator of image quality. The method is sensitive to the size of the structures present in the image (contrary to the contrast method, widely used to select the best images of a series) and can provide a quality map
    Giammanco, C.

    Advertised on:

    11
    2000
    Bibcode
    2000A&AS..147....1G
    Citations
    1
  • Refereed
    HST confirmation of the lensed quasar J03.13.
    In order to definitely prove the claim by Claeskens et al. (1996A&A...305L...9C) that J03.13 is a doubly imaged quasar, WFPC2 direct imaging and FOS spectroscopy of this compact system have been obtained with HST. These textbook case observations clearly show that J03.13 consists of two point-like images separated by 0.849"+/-0.001" with a
    Vanderriest, C. et al.

    Advertised on:

    11
    1997
    Bibcode
    1997A&A...327L...1S
    Citations
    19