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

  • Mapping the Youngest and Most Massive Stars in the Tarantula Nebula with MUSE-NFM
    The evolution of the most massive stars is a puzzle with many missing pieces. Statistical analyses are key to providing anchors to calibrate theory, but performing these studies is an arduous job. The state-of-the-art integral field spectrograph Multi Unit Spectroscopic Explorer (MUSE) has stirred up stellar astrophysicists, who are excited about
    Castro, N. et al.

    Fecha de publicación:

    3
    2021
    Número de citas
    6
  • Mapping stellar activity indicators across the M dwarf domain
    Despite stellar magnetic activity being present in most cool stars, its effects on spectroscopic observations are still not well understood. Several activity indicators are routinely used to identify activity-related signals in radial velocity (RV) measurements, but not all indicators trace exactly the same effects, nor are any of them always
    Lafarga, Marina et al.

    Fecha de publicación:

    3
    2021
    Número de citas
    0
  • Long-term evolution of three light bridges developed on the same sunspot
    One important feature of sunspots is the presence of light bridges. These structures are elongated and bright (as compared to the umbra) features that seem to be related to the formation and evolution of sunspots. In this work, we studied the long-term evolution and the stratification of different atmospheric parameters of three light bridges
    Griñón-Marín, A. B. et al.

    Fecha de publicación:

    3
    2021
    Número de citas
    8
  • Interstellar Extinction, Polarization, and Grain Alignment in the Sh 2-185 (IC 59 and IC 63) Region
    Optical and infrared continuum polarization from the interstellar medium is driven by radiative processes aligning the grains with the magnetic field. While a quantitative, predictive theory of radiative alignment torques (RATs) exists and has been extensively tested, several parameters of the theory remain to be fully constrained. In a recent
    Soam, Archana et al.

    Fecha de publicación:

    3
    2021
    Número de citas
    13
  • HIRES, the High-resolution Spectrograph for the ELT
    HIRES will be the high-resolution spectrograph at optical and near-infrared (NIR) wavelengths for ESO's Extremely Large Telescope (ELT). It will consist of three fibre-fed spectrographs providing a wavelength coverage of 0.4–1.8 µm (with a goal of 0.35–1.8 µm) at a spectral resolution of ~ 100 000. Fibre-feeding allows HIRES to have several
    Marconi, A. et al.

    Fecha de publicación:

    3
    2021
    Número de citas
    46
  • HARMONI: the ELT's First-Light Near-infrared and Visible Integral Field Spectrograph
    The High Angular Resolution Monolithic Optical and Near-infrared Integral field spectrograph (HARMONI) is the visible and near-infrared (NIR), adaptive-optics-assisted, integral field spectrograph for ESO's Extremely Large Telescope (ELT). It will have both a single-conjugate adaptive optics (SCAO) mode (using a single bright natural guide star)
    Thatte, N. et al.

    Fecha de publicación:

    3
    2021
    Número de citas
    29