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

  • The Missing Link? Discovery of Pulsations in the Nitrogen-rich PG 1159 Star PG 1144+005
    Up to 98% of all single stars will eventually become white dwarfs-stars that link the history and future evolution of the Galaxy, and whose previous evolution is engraved in their interiors. Those interiors can be studied using asteroseismology, utilizing stellar pulsations as seismic waves. The pulsational instability strips of DA and DB white
    Sowicka, Paulina et al.

    Fecha de publicación:

    9
    2021
    Número de citas
    9
  • The miniJPAS survey: A preview of the Universe in 56 colors
    The Javalambre-Physics of the Accelerating Universe Astrophysical Survey (J-PAS) will scan thousands of square degrees of the northern sky with a unique set of 56 filters using the dedicated 2.55 m Javalambre Survey Telescope (JST) at the Javalambre Astrophysical Observatory. Prior to the installation of the main camera (4.2 deg 2 field-of-view
    Bonoli, S. et al.

    Fecha de publicación:

    9
    2021
    Número de citas
    128
  • The lens SW05 J143454.4+522850: a fossil group at redshift 0.6?
    Fossil groups are considered the end product of natural galaxy group evolution in which group members sink towards the centre of the gravitational potential due to dynamical friction, merging into a single, massive, and X-ray bright elliptical. Since gravitational lensing depends on the mass of a foreground object, its mass concentration, and
    Denzel, Philipp et al.

    Fecha de publicación:

    9
    2021
    Número de citas
    0
  • The GAPS Programme at TNG. XXXI. The WASP-33 system revisited with HARPS-N
    Context. Giant planets in short-period orbits around bright stars represent optimal candidates for atmospheric and dynamical studies of exoplanetary systems. Aims: We aim to analyse four transits of WASP-33b observed with the optical high-resolution HARPS-N spectrograph to confirm its nodal precession, study its atmosphere, and investigate the
    Borsa, F. et al.

    Fecha de publicación:

    9
    2021
    Número de citas
    22
  • The Fornax3D project: Planetary nebulae catalogue and independent distance measurements to Fornax cluster galaxies
    Extragalactic planetary nebulae (PNe) offer a way to determine the distance to their host galaxies thanks to the nearly universal shape of the planetary nebulae luminosity function (PNLF). Accurate PNe distance measurements rely on obtaining well-sampled PNLFs and the number of observed PNe scales with the encompassed stellar mass. This means
    Spriggs, T. W. et al.

    Fecha de publicación:

    9
    2021
    Número de citas
    17
  • The EU Project NEOROCKS — NEO Rapid Observation, Characterization, and Key Simulations Project
    The knowledge of even some basic physical properties of a NEO such as the composition and the internal structure has strong implications for both science and impact mitigation. Depending on its composition and internal structure a meter-size object can completely burn in the atmosphere or reach the ground excavating an impact crater. To date, only
    Dotto, Elisabetta et al.

    Fecha de publicación:

    9
    2021
    Número de citas
    2