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

  • Understanding the Travel-time Asymmetry of Acoustic Waves in Sunspots with Time─Distance Helioseismology
    Mapping the subsurface structure and flow field of sunspots has been a challenging task for helioseismology. In this work, we investigate the propagation of acoustic waves in a sunspot in NOAA active region 11312 using time─distance helioseismology. Travel-times of waves traveling into and out of the sunspot are measured as functions of travel
    Li, Haiyu et al.

    Fecha de publicación:

    9
    2026
    Número de citas
    0
  • Three-dimensional Magnetic Field Structure of a Quiet-Sun Region Revealed by SUNRISE III/SCIP
    The balloon-borne stratospheric solar observatory SUNRISE III successfully completed 6.5 days of observations in 2024 July. One of its focal-plane instruments, the Sunrise Chromospheric Infrared spectroPolarimeter (SCIP), is a slit-scanning spectropolarimeter that simultaneously measures full Stokes profiles of multiple spectral lines in the 850 nm
    Kubo, Masahito et al.

    Fecha de publicación:

    9
    2026
    Número de citas
    2
  • The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry
    A wide range of variability mechanisms exist among intermediate-mass and massive stars, which are not yet fully understood. Using complementary data sources for a large population of B- and O-type stars, we aim to study the prevalence and interplay of different types of variability, including binarity, pulsation, and rotation, to prepare for future
    Thomson-Paressant, K. et al.

    Fecha de publicación:

    9
    2026
    Número de citas
    0
  • The Orbital Eccentricity─Radius Distribution for Warm, Single Planets in TESS
    We characterize the radius-dependent observed transiting eccentricity distribution of 219 warm (P = 8─50 days) systems with only one transiting planetary candidate identified during Sectors 1─69 of the Transiting Exoplanet Survey Satellite (TESS) mission. Using the "photoeccentric effect" in a hierarchical Bayesian framework, we first model the
    Fairnington, Tyler R. et al.

    Fecha de publicación:

    9
    2026
    Número de citas
    5
  • The Occurrence Rate of Nearby Planetary Companions to Hot Jupiters
    Of the >500 confirmed transiting hot Jupiters and ≈2000 additional candidates today, only 10 are known to have nearby companion planets. The survival of nearby companions means that these hot Jupiters cannot have migrated to their present location via dynamically disruptive high-eccentricity migration but instead have undergone disk migration or
    Sha, Lizhou et al.

    Fecha de publicación:

    9
    2026
    Número de citas
    19
  • The little blue and red dot Rosetta stones: Non-Gaussian broad lines, hot dust, and X-ray weakness
    The population of active galactic nuclei (AGNs) newly discovered by the James Webb Space Telescope (JWST) exhibits peculiar properties that distinguish it from both local type I AGNs and high-redshift quasars. Most of these sources are compact, appearing as `little dots'; among them, the sub-class (10-30% of the total) characterised by
    Brazzini, M. et al.

    Fecha de publicación:

    9
    2026
    Número de citas
    69