Tipo de publicación: Con árbitro

  • Publicación
    Activity at the Deuterium-burning Mass Limit in Orion
    We report very intense and variable Hα emission (pseudoequivalent widths of ~180 and 410 Å) of S Ori 55, a probable free-floating, M9-type substellar member of...
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    Activity from the Be/X-ray binary system V0332+53 during its intermediate-luminosity outburst in 2008
    Aims: We present a study of the Be/X-ray binary system V 0332+53 with the main goal of characterizing its behaviour mainly during the intermediate-luminosity X...
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    Activity of Comet 103P/Hartley 2 at the time of the EPOXI mission fly-by
    Comet 103P/Hartley 2 was observed on November 1-6, 2010, coinciding with the fly-by of the space probe EPOXI. The goal was to connect the large scale phenomena...
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    Activity of the Jupiter co-orbital comet P/2019 LD<SUB>2</SUB> (ATLAS) observed with OSIRIS at the 10.4 m GTC
    Context. The existence of comets with heliocentric orbital periods close to that of Jupiter (i.e., co-orbitals) has been known for some time. Comet 295P/LINEAR...
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    Ad orientem: Las iglesias románicas del Camino Francés en los reinos de Castilla y León bajo la perspectiva de la Astronomía Cultural*Ad orientem: Romanesque Churches of the French Way in the kingdoms of Castile and Leon from a Cultural Astronomy perspect
    RESUMEN: En este trabajo se examina, desde la perspectiva de la Astronomía Cultural, si las iglesias románicas del Camino de Santiago siguen un patrón de...
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    Adapting astronomical source detection software to help detect animals in thermal images obtained by unmanned aerial systems
    In this paper we describe an unmanned aerial system equipped with a thermal-infrared camera and software pipeline that we have developed to monitor animal...
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    Adaptive optics imaging and TAURUS 2-D spectroscopy of galaxy cores
    Many barred galaxies show enhanced star formation activity in ring-like regions around their centres, at typical radii of 1-2 kpc. We show how kinematic (WHT...
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    Adaptive optics near infrared integral field spectroscopy of NGC 2992
    Aims: NGC 2992 is an intermediate Seyfert 1 galaxy showing outflows on kilo parsec scales which might be due either to AGN or starburst activity. We therefore...
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    Adaptive optics parameters connection to wind speed at the Teide Observatory
    Current projects for large telescopes demand a proper knowledge of atmospheric turbulence to design efficient adaptive optics systems in order to reach large...