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 Western Bulge of 162173 Ryugu Formed as a Result of a Rotationally Driven Deformation Process
    162173 Ryugu, the target of Hayabusa2, is a spinning top-shaped asteroid. Observations by Optical Navigation Camera onboard Hayabusa2 have shown that the western side of this asteroid possesses a smooth surface and a sharp equatorial ridge, compared to the other side. Here, we propose that a rotationally-driven deformation process generated the
    Hirabayashi, Masatoshi et al.

    Fecha de publicación:

    9
    2019
    Número de citas
    0
  • The spectroscopic properties of the Lixiaohua Family, cradle of Main-Belt comets
    We present an analysis of the spectroscopic properties of the Lixiaohua asteroid family, which hosts two main-belt comets. This study will enhance our knowledge of how primitive asteroids were formed and the abundance of their water reservoir. Mapping the water abundance among the Solar System small body populations is a key constrain to understand
    De Pra, Mario et al.

    Fecha de publicación:

    9
    2019
    Número de citas
    0
  • The Sloan Digital Sky Survey as an Archetypal Mid-Scale Program
    We describe the Sloan Digital Sky Survey (SDSS) as an archetypal mid-scale program, including the technical, scientific, and organizational aspects underpinning its success over the last twenty years. Based on the SDSS experience, we present six recommendations that the funding mechanisms for mid-scale programs should be designed to ensure.
    Blanton, Michael et al.

    Fecha de publicación:

    9
    2019
    Número de citas
    0
  • The quantity of dark matter in early-type galaxies and its relation to the environment
    We study the behaviour of the dynamical and stellar mass inside the effective radius of early-type galaxies (ETGs) as a function of environment considering Newtonian dynamics, different surface-brightness profiles, different initial mass functions (IMF), and different redshift ranges. We use several samples of ETGs - ranging from 19 000 to 98 000
    Nigoche-Netro, A. et al.

    Fecha de publicación:

    9
    2019
    Número de citas
    5
  • The MASCARA and bRing photometric monitoring networks
    The MASCARA/bRing network consists of four separate observatories, located in La Palma, La Silla, Sutherland, and Siding Springs, and searches for exoplanet transits around bright stars. The three southern hemisphere stations allow for near continuous observations between the declination range of -30 to -90 degrees. These stations are sensitive to
    Dorval, Patrick et al.

    Fecha de publicación:

    9
    2019
    Número de citas
    0
  • The Magellanic System: the puzzle of the leading gas stream
    The Magellanic Clouds (MCs) are the most massive gas-bearing systems falling into the Galaxy at the present epoch. They show clear signs of interaction, manifested in particular by the Magellanic Stream, a spectacular gaseous wake that trails from the MCs extending more than 150° across the sky. Ahead of the MCs is the `Leading Arm' usually
    Tepper-García, Thor et al.

    Fecha de publicación:

    9
    2019
    Número de citas
    38