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

  • Influence of the magnetic cycle on the excitation of solar-like acoustic modes
    The Sun's convective envelope generates, by dynamo effect, a surface magnetic field whose strength evolves on an 11-year cycle, with a change in polarity at the end of each cycle. Similar activity cycles exist in other solar-type stars, influencing the stars' dynamics, including the properties of acoustic oscillations, which are excited by
    Panetier, Eva et al.

    Fecha de publicación:

    8
    2024
    Número de citas
    0
  • Hydrodynamic simulations of cool stellar atmospheres with MANCHA
    Context. Three-dimensional time-dependent simulations of stellar atmospheres are essential to study the surface of stars other than the Sun. These simulations require the opacity binning method to reduce the computational cost of solving the radiative transfer equation down to viable limits. The method depends on a series of free parameters, among
    Perdomo García, A. et al.

    Fecha de publicación:

    8
    2024
    Número de citas
    0
  • Hydrodynamic simulations of cool stellar atmospheres with MANCHA
    Context. Three-dimensional time-dependent simulations of stellar atmospheres are essential to study the surface of stars other than the Sun. These simulations require the opacity binning method to reduce the computational cost of solving the radiative transfer equation down to viable limits. The method depends on a series of free parameters, among
    Perdomo García, A. et al.

    Fecha de publicación:

    8
    2024
    Número de citas
    0
  • HD152843 b & c: the masses and orbital periods of a sub-Neptune and a superpuff Neptune
    We present the characterization of the two transiting planets around HD 152843 (TOI 2319, TIC 349488688) using an intensive campaign of HARPS-N radial velocities, and two sectors of TESS data. These data reveal a unique and fascinating system: HD 152843 b and c have near equal masses of around 9 $M_{\hbox{$\oplus $}}$ but differing radii of $3.05
    Nicholson, B. A. et al.

    Fecha de publicación:

    8
    2024
    Número de citas
    0
  • HARMONI at ELT: verification tests of opto-mechanical mounts for HARMONI preoptics in cryogenic environment
    HARMONI is the high angular optical and near-IR integral field spectrograph (IFS) for the ELT. The instrument covers a large spectral range from 470 to 2450nm with resolving powers from 3300 to 18000 and spatial sampling from 60 to 4mas. A workhorse instrument designed to operate in two Adaptive Optics modes - Single-Conjugate Adaptive Optics (SCAO
    Hernández-González, Alberto et al.

    Fecha de publicación:

    8
    2024
    Número de citas
    0
  • HARMONI at ELT: design and tests results of the instrument cryogenic fast shutter
    HARMONI is the first light visible and near-IR integral field spectrograph for the ELT. It covers a large spectral range from 470nm to 2450nm with resolving powers from 3300 to 18000 and spatial sampling from 60mas to 4mas. It can operate in two Adaptive Optics modes - SCAO (including a High Contrast capability) and LTAO - or with NOAO. The project
    Martín, Yolanda et al.

    Fecha de publicación:

    8
    2024
    Número de citas
    0