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

  • Binarity in the Central Stars of Planetary Nebulae and its Relationship to Stellar Evolution: An Observational Perspective
    The existing status of our knowledge of binary central stars of planetary nebulae will be explored. Binary modeling of known systems is providing physical parameters that can be compared amongst the sample, with nebular characteristics, and with similar binaries with no associated planetary nebula. Correlations among these areas will be discussed
    Hillwig, T. C. et al.

    Fecha de publicación:

    3
    2017
    Número de citas
    0
  • Bimodal regime in young massive clusters leading to subsequent stellar generations
    Massive stars in young massive clusters insert tremendous amounts of mass and energy into their surroundings in the form of stellar winds and supernova ejecta. Mutual shock-shock collisions lead to formation of hot gas, filling the volume of the cluster. The pressure of this gas then drives a powerful cluster wind. However, it has been shown that
    Wünsch, Richard et al.

    Fecha de publicación:

    3
    2017
    Número de citas
    2
  • Baade's window and APOGEE. Metallicities, ages, and chemical abundances
    Context. Baade's window (BW) is one of the most observed Galactic bulge fields in terms of chemical abundances. Owing to its low and homogeneous interstellar absorption it is considered the perfect calibration field for Galactic bulge studies. Aims: In the era of large spectroscopic surveys, calibration fields such as BW are necessary for cross
    Schultheis, M. et al.

    Fecha de publicación:

    3
    2017
    Número de citas
    71
  • B fields in OB stars (BOB): Concluding the FORS 2 observing campaign
    Aims: The B fields in OB stars (BOB) Collaboration is based on an ESO Large Programme to study the occurrence rate, properties, and ultimately the origin of magnetic fields in massive stars. Methods: In the framework of this program, we carried out low-resolution spectropolarimetric observations of a large sample of massive stars using FORS 2
    Schöller, M. et al.

    Fecha de publicación:

    3
    2017
    Número de citas
    71
  • Astrophysical applications of quasar microlensing
    We present a quick overview of several examples that illustrate the application of quasar microlensing to various problems of great interest in Astrophysics and Cosmology. We start introducing the main tool for simulating quasar microlensing, the magnification map. Then, the flux magnification statistics obtained from the magnification maps is used
    Mediavilla, E. et al.

    Fecha de publicación:

    3
    2017
    Número de citas
    0
  • Astronomy in towns? An archaeoastronomical approach to the Roman urbanism
    Although the final definition of Archaeoastronomy is still under debate, what is clear is that this discipline offers a different approach to the knowledge of ancient cultures than traditional archaeology has done so far. Archaeoastronomy considers the sky as an inseparabe part of the environment and thus an element of the transformed landscape
    Rodríguez-Antón, A. et al.

    Fecha de publicación:

    3
    2017
    Número de citas
    0