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

  • The dark side of galaxy stellar populations - II. The dependence of star-formation histories on halo mass and on the scatter of the main sequence
    Nearby galaxies are the end result of their cosmological evolution, which is predicted to be influenced by the growth of their host dark matter haloes. This co-evolution potentially leaves signatures in present-day observed galaxy properties, which might be essential to further understand how the growth and properties of galaxies are connected to
    Scholz-Díaz, Laura et al.

    Fecha de publicación:

    2
    2023
    Número de citas
    4
  • The galaxy size to halo spin relation of disc galaxies in cosmological hydrodynamical simulations
    In the standard disc galaxy formation model, the sizes of galactic discs are tightly related to the spin parameters λ of their dark matter haloes. The model has been wildly adopted by various semi-analytical galaxy formation models which have been extremely successful to interpret a large body of observational data. However, the size-λ correlation
    Yang, Hang et al.

    Fecha de publicación:

    2
    2023
    Número de citas
    14
  • The nature of 500 micron risers - II. Multiplicities and environments of sub-mm faint dusty star-forming galaxies
    We present Submillimeter Common User Bolometer Array 2 (SCUBA-2) and Submillimeter Array (SMA) follow-up observations of four candidate high-redshift dusty star-forming galaxies, selected as sources with rising spectral energy distributions in the 250, 350, and 500 μm Herschel SPIRE bands. Previous SMA observations showed no counterparts to these
    Cairns, J. et al.

    Fecha de publicación:

    2
    2023
    Número de citas
    1
  • Two decades of optical timing of the shortest-period binary star system HM Cancri
    The shortest-period binary star system known to date, RX J0806.3+1527 (HM Cancri), has now been observed in the optical for more than two decades. Although it is thought to be a double degenerate binary undergoing mass transfer, an early surprise was that its orbital frequency, f 0, is currently increasing as the result of gravitational wave
    Munday, James et al.

    Fecha de publicación:

    2
    2023
    Número de citas
    12
  • Two temperate Earth-mass planets orbiting the nearby star GJ 1002
    We report the discovery and characterisation of two Earth-mass planets orbiting in the habitable zone of the nearby M-dwarf GJ 1002 based on the analysis of the radial-velocity (RV) time series from the ESPRESSO and CARMENES spectrographs. The host star is the quiet M5.5 V star GJ 1002 (relatively faint in the optical, V ~ 13.8 mag, but brighter in
    Suárez Mascareño, A. et al.

    Fecha de publicación:

    2
    2023
    Número de citas
    20
  • Vortex Motions in the Solar Atmosphere
    Vortex flows, related to solar convective turbulent dynamics at granular scales and their interplay with magnetic fields within intergranular lanes, occur abundantly on the solar surface and in the atmosphere above. Their presence is revealed in high-resolution and high-cadence solar observations from the ground and from space and with state-of-the
    Tziotziou, K. et al.

    Fecha de publicación:

    2
    2023
    Número de citas
    11