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 deep narrowband survey for planetary nebulae at the outskirts of M 33
    Context. Planetary nebulae (PNe) are excellent tracers of stellar populations with low surface brightness, and therefore provide a powerful method to detect and explore the rich system of substructures discovered around the main spiral galaxies of the local group. Aim. We searched the outskirts of the local group spiral galaxy M 33 (the Triangulum)
    Galera-Rosillo, R. et al.

    Fecha de publicación:

    4
    2018
    Número de citas
    6
  • SPECTROSCOPIC AND PHOTOMETRIC CHARACTERIZATION OF PRIMITIVE ASTEROID COLLISIONAL FAMILIES
    The study of near-Earth asteroids (NEAs) is very important, due to three main reasons. First, they pose an impact risk for Earth, and damage produced by a possible collision will depend on the speed of the impact, the size of the object, and its composition. Second, given their proximity, they are easy access targets for the visit of space missions
    David Morate González

    Fecha de publicación:

    4
    2018
  • Three Small Planets Transiting a Hyades Star
    We present the discovery of three small planets transiting K2-136 (LP 358 348, EPIC 247589423), a late K dwarf in the Hyades. The planets have orbital periods of 7.9757 ± 0.0011, {17.30681}-0.00036+0.00034, and {25.5715}-0.0040+0.0038 {days}, and radii of 1.05 ± 0.16, 3.14 ± 0.36, and {1.55}-0.21+0.24 {R}\oplus , respectively. With an age of 600
    Livingston, J. H. et al.

    Fecha de publicación:

    3
    2018
    Número de citas
    53
  • The stellar orbit distribution in present-day galaxies inferred from the CALIFA survey
    Galaxy formation entails the hierarchical assembly of mass, along with the condensation of baryons and the ensuing, self-regulating star formation1,2. The stars form a collisionless system whose orbit distribution retains dynamical memory that can constrain a galaxy's formation history3. The orbits dominated by ordered rotation, with near-maximum
    Zhu, L. et al.

    Fecha de publicación:

    3
    2018
    Número de citas
    79
  • The Resolved Stellar Populations in the LEGUS Galaxies1
    The Legacy ExtraGalactic UV Survey (LEGUS) is a multiwavelength Cycle 21 Treasury program on the Hubble Space Telescope. It studied 50 nearby star-forming galaxies in 5 bands from the near-UV to the I-band, combining new Wide Field Camera 3 observations with archival Advanced Camera for Surveys data. LEGUS was designed to investigate how star
    Sabbi, E. et al.

    Fecha de publicación:

    3
    2018
    Número de citas
    88
  • The Metal-poor non-Sagittarius (?) Globular Cluster NGC 5053: Orbit and Mg, Al, and Si Abundances
    Metal-poor globular clusters (GCs) exhibit intriguing Al–Mg anti-correlations and possible Si–Al correlations, which are important clues to decipher the multiple-population phenomenon. NGC 5053 is one of the most metal-poor GCs in the nearby universe and has been suggested to be associated with the Sagittarius (Sgr) dwarf galaxy, due to its
    Tang, B. et al.

    Fecha de publicación:

    3
    2018
    Número de citas
    25