Publicaciones

Esta sección ofrece el acceso a la base de datos de Publicaciones que recopila los artículos del IAC publicados en revistas científicas. Por favor, pulsa la flecha del menú para ver todas las opciones de búsqueda y de ordenación de resultados; autor, revista, año, etc..

Además ofrece acceso al  repositorio de preprints del IAC: https://research.iac.es/preprints/l

  • Galactic archaeology for amateur astronomers: RR Lyrae stars as tracers of the Milky Way formation
    Cosmological models predict that large galaxies like the Milky Way formed from the accretion of smaller stellar systems. The most spectacular of these merger events are stellar tidal streams, rivers of stars and dark matter that envelop the discs of spiral galaxies. We present a research project for a collaboration with amateur astronomers in the
    Carballo-Bello, J. A. et al.

    Fecha de publicación:

    6
    2011
    Número de citas
    0
  • From nearby clusters to Fossil Groups. Clues through their luminosity functions
    Not Available
    Zarattini, Stefano

    Fecha de publicación:

    6
    2011
    Número de citas
    0
  • FOssil Group Origins (FOGO) project: a multiwavelenth view of fossil galaxy systems
    Not Available
    Aguerri, J. Alfonso L.

    Fecha de publicación:

    6
    2011
    Número de citas
    0
  • EPOXI: Comet 103P/Hartley 2 Observations from a Worldwide Campaign
    Earth- and space-based observations provide synergistic information for space mission encounters by providing data over longer timescales, at different wavelengths and using techniques that are impossible with an in situ flyby. We report here such observations in support of the EPOXI spacecraft flyby of comet 103P/Hartley 2. The nucleus is small
    Meech, K. J. et al.

    Fecha de publicación:

    6
    2011
    Número de citas
    106
  • Dynamics of early-type dwarf galaxies in the Virgo Cluster - a SAURON perspective
    Not Available
    Ryś, Agnieszka

    Fecha de publicación:

    6
    2011
    Número de citas
    0
  • Color-Magnitude Diagrams, Probabilistic Synthesis Models and the Upper Mass Limit of the Initial Mass Function
    We present the underlying relations between color-magnitude diagrams (CMDs) and synthesis models through the use of stellar luminosity distribution functions. CMD studies make direct use of the stellar luminosity distribution function while, in general, synthesis models only use its mean value, even though high-order moments can also be obtained
    Cerviño, M. et al.

    Fecha de publicación:

    6
    2011
    Número de citas
    4