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

  • Globular cluster systems and the origin of early-type dwarfs in Virgo
    Not Available
    Sánchez-Janssen, R. et al.

    Fecha de publicación:

    1
    2011
    Número de citas
    0
  • Global p-mode oscillations throughout the complete solar cycle 23 and the beginning of cycle 24
    The parameters of the p-mode oscillations vary with solar activity. Such temporal variations provide insights for the study of the structural and dynamical changes occurring in the Sun's interior throughout the solar cycle. We present here a complete picture of the temporal variations of the global p-mode parameters (excitation, damping, frequency
    Salabert, D. et al.

    Fecha de publicación:

    1
    2011
    Número de citas
    11
  • Exploring the connection of weak winds and magnetic fields
    The theory of radiatively driven winds successfully explains the key points of the stellar winds of hot massive stars. However, there is an apparent break-down of this paradigm at log L/L_&odot
    Garcia, Miriam et al.

    Fecha de publicación:

    1
    2011
    Número de citas
    2
  • Evolution of Brightest Cluster Galaxy Structural Parameters in the Last ~6 Gyr: Feedback Processes Versus Merger Events
    We present results on the evolution of the structural parameters of two samples of brightest cluster galaxies (BCGs) in the last 6 Gyr. The nearby sample of BCGs consists of 69 galaxies from the WINGS survey spanning a redshift range of 0.04 z 0.07. The intermediate-redshift (0.3 z 0.6) sample is formed by 20 BCGs extracted from the Hubble
    Ascaso, B. et al.

    Fecha de publicación:

    1
    2011
    Número de citas
    52
  • Evidence for Circumstellar Material in Type Ia Supernovae via Na I D Absorption Features
    Type Ia Supernovae (SNe Ia) have high and homogeneous luminosities, making them an essential tool for measuring distances on a cosmic scale, useful to gauge the geometry and evolution of the Universe. However, the nature of the progenitor system of these explosions is still uncertain. The consensus view is that SNe Ia originate from an accreting
    Sternberg, Assaf et al.

    Fecha de publicación:

    1
    2011
    Número de citas
    0