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/

  • Ionized Gas in Spiral Galaxies and the Ionization of the Intergalactic Medium
    Not Available
    Beckman, John E. et al.

    Advertised on:

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    1999
    Citations
    0
  • Internet resources for professional astronomy : proceedings of the IX Canary Islands Winter School of Astrophysics
    This book presents a comprehensive guide to the impact of the internet on professional astronomy. Each chapter deals with a range of the electromagnetic spectrum, with authors first discussing the corresponding problems for each range, particularly those that can be treated by access to very large databases. They then describe how data and
    Kidger, Mark R. et al.

    Advertised on:

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    1999
    Citations
    2
  • Influence of unresolved optically-thin irregularities on quiet Sun magnetic field determinations.
    Not Available
    Almeida, J.

    Advertised on:

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    1999
    Citations
    0
  • Influence of Unresolved Optically-Thin Irregularities on Quiet Sun Magnetic Field Determinations
    Observations and theory both point out that the magnetic photosphere is not smooth but irregular at optically-thin scales. The relevance of these irregularities for a proper magnetic field diagnostics depends upon the not yet known structure of the magnetic field fluctuations (and, of course, on the purpose of our determination). Sánchez Almeida &
    Sánchez Almeida, J.

    Advertised on:

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    1999
    Citations
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  • Implementation of a Filter for the Restoration of Solar Granulation Images
    Not Available
    Sánchez Cuberes, M. et al.

    Advertised on:

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    1999
    Citations
    1
  • How Binary Stars affect Galactic Chemical Evolution
    At least 60% of stars appear to be binary and about half of these are close enough to interact. Because of the enormous expansion on the AGB, many of these interactions will involve an AGB star and a relatively compact companion, anything from a low-mass main-sequence star to a degenerate remnant. Mass loss plays the dominant role in determining
    Tout, C. A. et al.

    Advertised on:

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    1999
    Citations
    2