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

  • An enhanced slope in the transmission spectrum of the hot Jupiter WASP-104b
    We present the optical transmission spectrum of the hot Jupiter WASP-104b based on one transit observed by the blue and red channels of the Double Spectrograph (DBSP) at the Palomar 200-inch telescope and 14 transits observed by the MuSCAT2 four-channel imager at the 1.52-m Telescopio Carlos Sánchez. We also analyse 45 additional K2 transits, after
    Chen, G. et al.

    Fecha de publicación:

    1
    2021
    Número de citas
    17
  • A prediction about the age of thick discs as a function of the stellar mass of the host galaxy
    One of the suggested thick disc formation mechanisms is that they were born quickly and in situ from a turbulent clumpy disc. Subsequently, thin discs formed slowly within them from leftovers of the turbulent phase and from material accreted through cold flows and minor mergers. In this Letter, I propose an observational test to verify this
    Comerón, S.

    Fecha de publicación:

    1
    2021
    Número de citas
    5
  • A planetary system with two transiting mini-Neptunes near the radius valley transition around the bright M dwarf TOI-776
    We report the discovery and characterization of two transiting planets around the bright M1 V star LP 961-53 (TOI-776, J = 8.5 mag, M = 0.54 ± 0.03 M ☉) detected during Sector 10 observations of the Transiting Exoplanet Survey Satellite (TESS). Combining the TESS photometry with HARPS radial velocities, as well as ground-based follow-up transit
    Luque, R. et al.

    Fecha de publicación:

    1
    2021
    Número de citas
    46
  • 2D kinematics of massive stars near the Galactic Centre
    The presence of massive stars (MSs) in the region close to the Galactic Centre (GC) poses several questions about their origin. The harsh environment of the GC favours specific formation scenarios, each of which should imprint characteristic kinematic features on the MSs. We present a 2D kinematic analysis of MSs in a GC region surrounding Sgr A*
    Libralato, Mattia et al.

    Fecha de publicación:

    1
    2021
    Número de citas
    27
  • What Equinox?
    Equinox, what a controversial concept! Since the dawn of archaeoastronomy this has arguably been the most problematic concept—perhaps together with the lunar standstills or lunistices (González García and Belmonte, Journal of Skyscape Archaeology, 5(2):178-190, 2019)—to be taken into account since it was first used in `megalithic' astronomy to
    Belmonte, Juan Antonio

    Fecha de publicación:

    0
    2021
    Número de citas
    1
  • Thermally altered subsurface material of asteroid (162173) Ryugu
    Analyses of meteorites and theoretical models indicate that some carbonaceous near-Earth asteroids may have been thermally altered due to radiative heating during close approaches to the Sun 1-3. However, the lack of direct measurements on the subsurface doesn't allow us to distinguish thermal alteration due to radiative heating from parent-body
    Kitazato, K. et al.

    Fecha de publicación:

    0
    2021
    Número de citas
    56