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

  • AGN feedback and the origin and fate of the hot gas in early-type galaxies
    We present the results of two-dimensional, grid-type hydrodynamical simulations, with parsec-scale central resolution, for the evolution of the hot gas in isolated early-type galaxies (ETGs). The simulations include a physically self-consistent treatment of the mechanical (from winds) and radiative AGN feedback, and were run for a large set of
    Pellegrini, Silvia et al.

    Fecha de publicación:

    0
    2020
    Número de citas
    0
  • A MUSE study of the fast bar in the weakly-interacting galaxy NGC 4264
    We present surface photometry and stellar kinematics of NGC 4264, a lenticular galaxy in the region of the Virgo Cluster undergoing a tidal interaction with its neighbour, NGC 4261. We measured the bar radius and strength from SDSS imaging and the bar pattern speed from MUSE integral-field spectroscopy. We find that NGC 4264 hosts a strong and
    Cuomo, Virginia et al.

    Fecha de publicación:

    0
    2020
    Número de citas
    1
  • 3D asymmetrical kinematics of mono-age populations from LAMOST and Gaia common red clump stars
    With the LAMOST DR4 and Gaia DR2 common red clump giant stars, we investigate the three-dimensional kinematics of Milky Way disk stars in mono-age populations between Galactocentric distances of R = 6 and 15 kpc. We confirm the 3D asymmetrical motions of recent works, and provide time tagging of the Galactic outer disk asymmetrical motions. Radial
    Wang, H. -F. et al.

    Fecha de publicación:

    0
    2020
    Número de citas
    20
  • The Impact of a Fossil Magnetic Field on Dipolar Mixed-Mode Frequencies in Sub- and Red-Giant Stars
    The recent discovery of low-amplitude dipolar oscillation mixed modes in massive red giants indicates the presence of a missing physical process inside their cores. Stars more massive than ∼ 1.3 M ☉ are known to develop a convective core during the main-sequence: the dynamo process triggered by this convection could be the origin of a strong
    Bugnet, L. et al.

    Fecha de publicación:

    2020
    Número de citas
    0
  • Surface Rotation and Magnetic Activity of Solar-Like Stars: Impact on Seismic Detections
    Rotation plays an important role in the evolution of stars. For decades rotation-age relationships have been used as surface rotation can be measured rather easily. Here we show the result of the measurement of rotation periods for a large number of Kepler solar-like stars along with their level of magnetic activity. We also study solar-like stars
    Mathur, S. et al.

    Fecha de publicación:

    2020
    Número de citas
    1
  • Open Discussion
    During the last morning of the conference, a one-hour open discussion allowed the participants to debate some of the "hot" topics presented all along the meeting as well as on some of the key issues in the field mostly related with the work Prof. Michael J. Thompson studied during his carrier. The discussion covered theory and methods, current and
    García, R. A. et al.

    Fecha de publicación:

    2020
    Número de citas
    0