Tipo de publicación: Con árbitro

  • Publicación
    The dust morphology of the elliptical Galaxy M 86 with SPIRE
    We present Herschel-SPIRE observations at 250-500 μm of the giant elliptical galaxy M 86 and examine the distribution of the resolved cold dust emission and its...
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    The dust tail of Comet C/1999 T1 McNaught-Hartley
    A numerical method to compute cometary dust tail brightnesses has been developed. The method, analogous in many ways to the inverse Monte Carlo method proposed...
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    The dust-gas AGN torus as constrained from X-ray and mid-infrared observations
    Context. In recent decades, several multiwavelength studies have been dedicated to exploring the properties of the obscuring material in active galactic nuclei...
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    The dusty tori of nearby QSOs as constrained by high-resolution mid-IR observations
    We present mid-infrared (MIR; 7.5-13.5 μm) imaging and spectroscopy observations obtained with the CanariCam (CC) instrument on the 10.4-m Gran Telescopio...
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    The dwarf galaxy population in nearby clusters from the KIWICS survey
    We analyse a sample of 12 galaxy clusters, from the Kapteyn IAC WEAVE INT Cluster Survey (KIWICS) looking for dwarf galaxy candidates. By using photometric data...
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    The dynamic magnetic quiet Sun: physical mechanisms and UV signature
    The changes in the Sun occurring at human time-scales can be pinned down to the presence of magnetic fields. These fields determine the structure of the outer...
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    The dynamical and chemical evolution of dwarf spheroidal galaxies
    We present a large sample of fully self-consistent hydrodynamical Nbody/Tree-SPH simulations of isolated dwarf spheroidal galaxies (dSphs). It has enabled us to...
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    The Dynamical Evolution of Planetary Nebulae after the Fast Wind
    We explore the dynamics of ionization-bounded planetary nebulae after the termination of the fast stellar wind. When the stellar wind becomes negligible, the...
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    The Dynamical Evolution of the Circumstellar Gas around Low- and Intermediate-Mass Stars. I. The Asymptotic Giant Branch
    We have investigated the dynamical interaction of low- and intermediate-mass stars (from 1 to 5 Msolar) with their interstellar medium (ISM). In this first...