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

  • A calibration point for stellar evolution from massive star asteroseismology
    Massive stars are progenitors of supernovae, neutron stars and black holes. During the hydrogen-core burning phase, their convective cores are the prime drivers of their evolution, but inferences of core masses are subject to unconstrained boundary mixing processes. Moreover, uncalibrated transport mechanisms can lead to strong envelope mixing and
    Burssens, Siemen et al.

    Fecha de publicación:

    8
    2023
    Número de citas
    45
  • A broadband thermal emission spectrum of the ultra-hot Jupiter WASP-18b
    Close-in giant exoplanets with temperatures greater than 2,000 K (`ultra-hot Jupiters') have been the subject of extensive efforts to determine their atmospheric properties using thermal emission measurements from the Hubble Space Telescope (HST) and Spitzer Space Telescope 1-3. However, previous studies have yielded inconsistent results because
    Coulombe, Louis-Philippe et al.

    Fecha de publicación:

    8
    2023
    Número de citas
    117
  • A Bayesian estimation of the Milky Way's circular velocity curve using Gaia DR3
    Aims: Our goal is to calculate the circular velocity curve of the Milky Way, along with corresponding uncertainties that quantify various sources of systematic uncertainty in a self-consistent manner. Methods: The observed rotational velocities are described as circular velocities minus the asymmetric drift. The latter is described by the radial
    Põder, Sven et al.

    Fecha de publicación:

    8
    2023
    Número de citas
    14
  • A 5.3-min-period pulsing white dwarf in a binary detected from radio to X-rays
    White dwarf stars are the most common stellar fossils. When in binaries, they make up the dominant form of compact object binary within the Galaxy and can offer insight into different aspects of binary formation and evolution. One of the most remarkable white dwarf binary systems identified to date is AR Scorpii (AR Sco). AR Sco is composed of an M
    Pelisoli, Ingrid et al.

    Fecha de publicación:

    8
    2023
    Número de citas
    49
  • X-Shooting ULLYSES: Massive stars at low metallicity. I. Project description
    Observations of individual massive stars, super-luminous supernovae, gamma-ray bursts, and gravitational wave events involving spectacular black hole mergers indicate that the low-metallicity Universe is fundamentally different from our own Galaxy. Many transient phenomena will remain enigmatic until we achieve a firm understanding of the physics
    Vink, Jorick S. et al.

    Fecha de publicación:

    7
    2023
    Número de citas
    56
  • VaTEST. II. Statistical Validation of 11 TESS-detected Exoplanets Orbiting K-type Stars
    NASA's Transiting Exoplanet Survey Satellite (TESS) is an all-sky survey mission designed to find transiting exoplanets orbiting nearby bright stars. It has identified more than 329 transiting exoplanets, and almost 6000 candidates remain unvalidated. In this manuscript, we discuss the findings from the ongoing Validation of Transiting Exoplanets
    Mistry, Priyashkumar et al.

    Fecha de publicación:

    7
    2023
    Número de citas
    9