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

  • Star-forming galaxies at low-redshift in the SHARDS survey
    Context. The physical processes driving the evolution of star formation (SF) in galaxies over cosmic time still present many open questions. Recent galaxy surveys allow now to study these processes in great detail at intermediate redshift (0 ≤ z ≤ 0.5). Aims: We build a complete sample of star-forming galaxies and analyze their properties, reaching
    Lumbreras-Calle, A. et al.

    Fecha de publicación:

    1
    2019
    Número de citas
    14
  • Spiral-shaped wavefronts in a sunspot umbra
    Context. Solar active regions show a wide variety of oscillatory phenomena. The presence of the magnetic field leads to the appearance of several wave modes whose behavior is determined by the sunspot thermal and magnetic structure. Aims: We aim to study the relation between the umbral and penumbral waves observed at the high photosphere and the
    Felipe, T. et al.

    Fecha de publicación:

    1
    2019
    Número de citas
    16
  • SPECTROSCOPIC AND PHYSICAL CHARACTERIZATION OF THE GALACTIC O-TYPE STARS TARGETED BY THE IACOB & OWN SURVEYS
    Las estrellas O representan una fase fundamental en el zoológico de las estrellas masivas. Ionizan el material a su alrededor e inundan su entorno con material procesado a través de fuertes vientos estelares y explosiones de supernova. Además de la pérdida de masa, factores como la rotación y la multiplicidad (así como la interacción entre ellos)
    Gonzalo Holgado Alijo

    Fecha de publicación:

    1
    2019
  • Spectro-polarimetric analysis of a short lived solar active region
    The physical processes related to the formation, evolution and disappearance of solar active regions are not completely clear. High-resolution solar spectro-polarimetric data are needed to investigate these processes with unprecedented details. Here we present the analysis of the short-lived NOAA 12549 active region using high-resolution spectro
    Viavattene, G. et al.

    Fecha de publicación:

    1
    2019
    Número de citas
    0
  • Space astrometry of the very massive ˜150 M⊙ candidate runaway star VFTS682
    How very massive stars form is still an open question in astrophysics. VFTS682 is among the most massive stars known, with an inferred initial mass of ≳150 M_⊙. It is located in 30 Doradus at a projected distance of 29 pc from the central cluster R136. Its apparent isolation led to two hypotheses: either it formed in relative isolation or it was
    Renzo, M. et al.

    Fecha de publicación:

    1
    2019
    Número de citas
    17
  • Software architecture of the high-level control of FRIDA
    FRIDA (inFRared Imager and Dissector for Adaptive optics) is a near-infrared integral-field spectrograph operating at the wavelength range of 0.9 to 2.5 μm for use at the Nasmyth B platform of the Gran Telescopio de Canarias (GTC). FRIDA is a collaborative project led by the Instituto de Astronomía Universidad Nacional Autónoma de México (IA-UNAM
    Guzmán Alvaréz, C. et al.

    Fecha de publicación:

    1
    2019
    Número de citas
    1