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

  • Two-dimensional simulations of coronal rain dynamics. I. Model consisting of a vertical magnetic field and an unbounded atmosphere
    Context. Coronal rain often comes about as the final product of evaporation and condensation cycles that occur in active regions. Observations show that the condensed plasma falls with an acceleration that is less than that of free fall. Aims: We aim to improve the understanding of the physical mechanisms behind the slower than free-fall motion and
    Martínez-Gómez, D. et al.

    Fecha de publicación:

    2
    2020
    Número de citas
    14
  • Two Ultra-faint Milky Way Stellar Systems Discovered in Early Data from the DECam Local Volume Exploration Survey
    We report the discovery of two ultra-faint stellar systems found in early data from the DECam Local Volume Exploration survey (DELVE). The first system, Centaurus I (DELVE J1238─4054), is identified as a resolved overdensity of old and metal-poor stars with a heliocentric distance of ${\text{}}{D}_{\odot }={116.3}_{-0.6}^{+0.6}\,\mathrm{kpc}$ , a
    Mau, S. et al.

    Fecha de publicación:

    2
    2020
    Número de citas
    74
  • Trojans in the Solar Neighborhood
    About 20% of stars in the solar vicinity are in the Hercules stream, a bundle of stars that move together with a velocity distinct from the Sun. Its origin is still uncertain. Here, we explore the possibility that Hercules is made of trojans, stars captured at L4, one of the Lagrangian points of the stellar bar. Using GALAKOS─a high-resolution N
    D'Onghia, Elena et al.

    Fecha de publicación:

    2
    2020
    Número de citas
    42
  • Tracking Downflows from the Chromosphere to the Photosphere in a Solar Arch Filament System
    We study the dynamics of plasma along the legs of an arch filament system (AFS) from the chromosphere to the photosphere, observed with high-cadence spectroscopic data from two ground-based solar telescopes: the GREGOR telescope (Tenerife) using the GREGOR Infrared Spectrograph in the He i 10830 Å range and the Swedish Solar Telescope (La Palma)
    González Manrique, Sergio Javier et al.

    Fecha de publicación:

    2
    2020
    Número de citas
    4
  • Thermal emission from the amorphous dust: An alternative possibility of the origin of the anomalous microwave emission
    Complete studies of the radiative processes of thermal emission from the amorphous dust from microwave through far-infrared wavebands are presented by taking into account, self-consistently for the first time, the standard two-level systems (TLS) model of amorphous materials. The observed spectral energy distributions (SEDs) for the Perseus
    Nashimoto, Masashi et al.

    Fecha de publicación:

    2
    2020
    Número de citas
    6
  • The young massive SMC cluster NGC 330 seen by MUSE. I. Observations and stellar content
    Context. A majority of massive stars are part of binary systems, a large fraction of which will inevitably interact during their lives. Binary-interaction products (BiPs), that is, stars affected by such interaction, are expected to be commonly present in stellar populations. BiPs are thus a crucial ingredient in the understanding of stellar
    Bodensteiner, J. et al.

    Fecha de publicación:

    2
    2020
    Número de citas
    39