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

  • Surface abundances of CNO in Galactic O-stars: a pilot study with FASTWIND
    Context. Rotational mixing is known to significantly affect the evolution of massive stars; however, we still lack a consensus regarding the various possible modeling approaches and mixing recipes describing this process. The empirical investigation of surface abundances of carbon, nitrogen, and oxygen (CNO) in large samples of O- and B-type stars
    Carneiro, L. P. et al.

    Fecha de publicación:

    3
    2019
    Número de citas
    14
  • Stellar atmospheric parameters of FGK-type stars from high-resolution optical and near-infrared CARMENES spectra
    With the aim of using classic spectroscopic methods with high resolution and high signal-to-noise ratio in the NIR spectral window, we made a selection of 66 FGK-type stars observed with CARMENES, the brand-new, ultra-stable, double-channel spectrograph at the Spanish-German 3.5m Calar Alto telescope. These spectra are part of a CARMENES stellar
    Marfil, E. et al.

    Fecha de publicación:

    3
    2019
    Número de citas
    1
  • Star formation and gas in the minor merger UGC 10214
    Minor mergers play a crucial role in galaxy evolution. UGC 10214 (the Tadpole galaxy) is a prime example of this process in which a dwarf galaxy has interacted with a large spiral galaxy ˜250 Myr ago and produced a perturbed disc and a giant tidal tail. We used a multi-wavelength dataset that partly consists of new observations (Hα, HI, and CO) and
    Rosado-Belza, D. et al.

    Fecha de publicación:

    3
    2019
    Número de citas
    2
  • Spectral synthesis of CARMENES M-type stars: stellar atmospheric parameters
    We show our very first results regarding the stellar atmospheric parameter determinations (T_{eff} , log g, [Fe/H]) of M-type stars observed with CARMENES te{Carmenes} by means of the spectral synthesis method. We have selected spectral ranges around iron and titanium lines and molecular bands in three reference M-type stars: GX And (M1.0 V)
    Lázaro, F. J. et al.

    Fecha de publicación:

    3
    2019
    Número de citas
    1
  • Spectral energy distributions and luminosities of M dwarfs in the CARMENES search for exoplanets
    In the quest for Earth-sized exoplanets, M dwarfs are stars of increasing interest during the last two decades. Their small sizes and masses as compared to our Sun make them specially suitable targets to look for the signatures of planetary companions, as their habitable zones fall closer to their host star. Despite being the most abundant stars in
    Cifuentes, C. et al.

    Fecha de publicación:

    3
    2019
    Número de citas
    0
  • Space developments at IACTec
    IACTec is a technological and business space created by the Instituto de Astrofísica de Canarias (IAC) to promote collaboration between the public and private sectors. Our objective is to foster the creation of quality employment and the generation of value-added technological products with high marketing potential, both nationally and
    Oscoz, A. et al.

    Fecha de publicación:

    3
    2019
    Número de citas
    0