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

  • Venus Atmospheric Zonal Winds from Contemporaneous Akatsuki UVI and IRTF/SpeX 2.3 µm Images
    We compare Venus dayside cloud top winds from Akatsuki UVI images to contemporaneous winds in the lower clouds retrieved on the night side using IRTF/SpeX 2.3 µm images. From Nov 19 to Dec 6, 2018, we obtained daily images of the night side of Venus with SpeX at 1.74, 2.3 and 5.1 µm, and spectral images cubes of the disk from 0.7 to 2.5 µm. On Nov
    Bullock, M. A. et al.

    Fecha de publicación:

    10
    2020
    Número de citas
    0
  • Ubiquitous hundred-Gauss magnetic fields in solar spicules
    Aims: We aim to study the magnetic field in solar spicules using high-resolution spectropolarimetric observations in the Ca II 8542 Å line obtained with the Swedish 1-m Solar Telescope. Methods: The equations that result from the application of the weak field approximation (WFA) to the radiative transfer equations were used to infer the line-of
    Kriginsky, M. et al.

    Fecha de publicación:

    10
    2020
    Número de citas
    9
  • Tracing the evolution of dust-obscured activity using sub-millimetre galaxy populations from STUDIES and AS2UDS
    We analyse the physical properties of 121 SNR ≥ 5 sub-millimetre galaxies (SMGs) from the STUDIES 450 μm survey. We model their UV-to-radio spectral energy distributions using MAGPHYS+photo-z and compare the results to similar modelling of 850 μm-selected SMG sample from AS2UDS, to understand the fundamental physical differences between the two
    Dudzevičiūtė, U. et al.

    Fecha de publicación:

    10
    2020
    Número de citas
    0
  • The S2 stream: the shreds of a primitive dwarf galaxy
    The S2 stream is a kinematically cold stream that is plunging downwards through the Galactic disc. It may be part of a hotter and more diffuse structure called the Helmi stream. We present a multi-instrument chemical analysis of the stars in the metal-poor S2 stream using both high- and low-resolution spectroscopy, complemented with a re-analysis
    Aguado, David S. et al.

    Fecha de publicación:

    10
    2020
    Número de citas
    0
  • The principle of maximum entropy explains the cores observed in the mass distribution of dwarf galaxies
    Cold dark matter (CDM) simulations predict a central cusp in the mass distribution of galaxies. This prediction is in stark contrast with observations of dwarf galaxies that show a central plateau or "core" in their density distribution. The proposed solutions to this core-cusp problem can be classified into two types. One invokes feedback
    Sánchez Almeida, Jorge et al.

    Fecha de publicación:

    10
    2020
    Número de citas
    12
  • The post-common-envelope binary central star of the planetary nebula PN G283.7-05.1. A possible post-red-giant-branch planetary nebula central star
    We present the discovery and characterisation of the post-common-envelope central star system in the planetary nebula PN G283.7-05.1. Deep images taken as part of the POPIPlaN survey indicate that the nebula may possess a bipolar morphology similar to other post-common-envelope planetary nebulae. Simultaneous light and radial velocity curve
    Jones, D. et al.

    Fecha de publicación:

    10
    2020
    Número de citas
    19