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 origin of the most luminous planetary nebulae: M31
    The Planetary Nebulae Luminosity Function (PNLF) is an important standard candle on the extragalactic distance ladder. Its use is based on the empirical evidence that the [OIII]5007Å luminosity of PNe reaches a maximum value, M*, invariant with galaxy type and with a small dependence on metallicity. The PNLF method, applied to more than 50 galaxies
    Galera-Rosillo, R. et al.

    Fecha de publicación:

    3
    2019
    Número de citas
    0
  • The missing mass conundrum of post-common-envelope planetary nebulae
    Most planetary nebulae (PNe) show beautiful, axisymmetric morphologies despite their progenitor stars being essentially spherical. Angular momentum provided by a close binary companion is widely invoked as the main agent that would help eject an axisymmetric nebula, after a brief phase of engulfment of the secondary within the envelope of the
    Santander-García, M. et al.

    Fecha de publicación:

    3
    2019
    Número de citas
    2
  • The longest stellar dance inside a planetary nebula
    The importance of long-period binaries for the formation and evolution of planetary nebulae is still rather poorly understood, which in part is due to the lack of central star systems that are known to comprise such long-period binaries. Here, we report on the latest results from the on-going Mercator-HERMES survey for variability in the central
    Jones, D.

    Fecha de publicación:

    3
    2019
    Número de citas
    0
  • The kinematics of local thick discs do not support an accretion origin⋆
    Thick discs are nearly ubiquitous components of the discs of present-day galaxies. It has been proposed that a fraction of their stars have been accreted. Here, we aim to find whether accretion of satellites is the main formation mechanism of thick discs. To do so, we observed a sample of eight nearby edge-on galaxies with the Multi-Unit
    Comerón, S. et al.

    Fecha de publicación:

    3
    2019
    Número de citas
    30
  • The GTC Adaptive Optics system: the high spatial resolution Adaptive Optics facility at GTC
    The GTC Adaptive Optics (GTCAO) system is the general Adaptive Optics facility that will provide diffraction limited images in the near-infrared to the GTC telescope. At Day 1 it will consist of a single deformable mirror with 21×21 actuators (373 useful actuators), conjugated to the telescope pupil and a Shack-Hartmann wavefront sensor with 20×20
    Béjar, V. J. S. et al.

    Fecha de publicación:

    3
    2019
    Número de citas
    1
  • The Fornax Deep Survey with the VST. V. Exploring the faintest regions of the bright early-type galaxies inside the virial radius
    Context. This paper is based on the multi-band (ugri) Fornax Deep Survey (FDS) with the VLT Survey Telescope (VST). We study bright early-type galaxies (mB ≤ 15 mag) in the 9 square degrees around the core of the Fornax cluster, which covers the virial radius (Rvir ˜ 0.7 Mpc). Aims: The main goal of the present work is to provide an analysis of the
    Iodice, E. et al.

    Fecha de publicación:

    3
    2019
    Número de citas
    68