Tipo de publicación: Con árbitro

  • Publicación
    Advection and dispersal of small magnetic elements in the very quiet Sun
    We track small magnetic structures on very quiet regions (internetwork) of the Sun. We follow the footpoints of small-scale magnetic loops that appear on the...
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    Adventures of a tidally induced bar
    Using N-body simulations, we study the properties of a bar induced in a discy dwarf galaxy as a result of tidal interaction with the Milky Way. The bar forms at...
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    Aerosols and Water Ice in Jupiter’s Stratosphere from UV-NIR Ground-based Observations
    Jupiter’s atmosphere has been sounded in transmission from the UV to the IR, as if it were a transiting exoplanet, by observing Ganymede while passing through...
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    AGB dust and gas ejecta in extremely metal-poor environments
    We present asymptotic giant branch (AGB) models of metallicity Z = 10-4 and 3 × 10-4, with the aim of understanding how the gas enrichment and the dust...
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    AGB Stars and Their Circumstellar Envelopes. I. the VULCAN Code
    The interplay between AGB interiors and their outermost layers, where molecules and dust form, is a problem of high complexity. As a consequence, physical...
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    AGB Stars and Their Circumstellar Envelopes: An Operative Approach to Computing Their Atmospheres
    The study of AGB stars necessarily covers a wide range of topics, from the primary astronomical observations to their interpretation in terms of fundamental...
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    AGB stars in the SMC: evolution and dust properties based on Spitzer observations
    We study the population of asymptotic giant branch (AGB) stars in the Small Magellanic Cloud (SMC) by means of full evolutionary models of stars of mass 1 M⊙ ≤...
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    AGC 226178 and NGVS 3543: Two Deceptive Dwarfs toward Virgo
    The two sources AGC 226178 and NGVS 3543, an extremely faint, clumpy, blue stellar system and a low surface brightness dwarf spheroidal, are adjacent systems in...
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    Age and helium content of the open cluster NGC 6791 from multiple eclipsing binary members. II. Age dependencies and new insights
    Context. Models of stellar structure and evolution can be constrained by measuring accurate parameters of detached eclipsing binaries in open clusters. Multiple...