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..

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  • V404 CYG/GS 2023+338: Monitoring in the Optical with Robotic Telescopes of the MASTER Global Network during the 2015 Superburst
    2070 unique, homogeneous photometric and polarization observations of the microquasar in a binary system with a black hole V404 Cyg/GS2023+338 obtained in 2015 with the MASTER global network of robotic telescopes (16 robotic telescopes located at eight points on the Earth in Russia, Spain, South Africa, and Argentina) are presented. MASTER was the
    Lipunov, V. M. et al.

    Fecha de publicación:

    7
    2019
    Número de citas
    2
  • Unveiling the 100 pc scale nuclear radio structure of NGC 6217 with e-MERLIN and the VLA
    We present high-sensitivity 1.51 GHz e-MERLIN (e-Multi-Element Radio-Linked Interferometer Network) radio images of the nearby galaxy NGC 6217. We resolve the compact radio source at the centre of NGC 6217 for the first time, finding a twin-lobed structure with a total linear size of ˜4 arcsec (˜400 pc). The radio source does not have a compact
    Williams, D. R. A. et al.

    Fecha de publicación:

    7
    2019
    Número de citas
    8
  • UNIT project: Universe N-body simulations for the Investigation of Theoretical models from galaxy surveys
    We present the UNIT N-body cosmological simulations project, designed to provide precise predictions for non-linear statistics of the galaxy distribution. We focus on characterizing statistics relevant to emission line and luminous red galaxies in the current and upcoming generation of galaxy surveys. We use a suite of precise particle mesh
    Chuang, Chia-Hsun et al.

    Fecha de publicación:

    7
    2019
    Número de citas
    84
  • Uncovering the birth of the Milky Way through accurate stellar ages with Gaia
    Knowledge of the ages of the stars formed over a galaxy's lifetime is fundamental to an understanding of its formation and evolution. However, stellar ages are difficult to obtain since they cannot be measured from observations, but require comparison with stellar models 1. Alternatively, age distributions can be derived by applying the robust
    Gallart, Carme et al.

    Fecha de publicación:

    7
    2019
    Número de citas
    233
  • Ultra-bright CO and [{\rm{C}}\,{\rm{I}}] Emission in a Lensed z = 2.04 Submillimeter Galaxy with Extreme Molecular Gas Properties
    We report the very bright detection of cold molecular gas with the IRAM NOEMA interferometer of the strongly lensed source WISE J132934.18+224327.3 at z = 2.04, the so-called Cosmic Eyebrow. This source has a similar spectral energy distribution from optical-mid/IR to submillimeter/radio but significantly higher fluxes than the well-known lensed
    Dannerbauer, H. et al.

    Fecha de publicación:

    7
    2019
    Número de citas
    31
  • Two-fluid simulations of waves in the solar chromosphere. I. Numerical code verification
    Solar chromosphere consists of a partially ionized plasma, which makes modeling the solar chromosphere a particularly challenging numerical task. Here we numerically model chromospheric waves using a two-fluid approach with a newly developed numerical code. The code solves two-fluid equations of conservation of mass, momentum, and energy, together
    Popescu Braileanu, B. et al.

    Fecha de publicación:

    7
    2019
    Número de citas
    53