Tipo de publicación: Sin árbitro

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    Strong lithium lines in red supergiants at different metallicities
    Current models of stellar evolution predict that stars more massive than ∼6 M ⊙ should have completely depleted all lithium (Li) in their atmospheres by the...
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    Strong Size Evolution of the Most Massive Galaxies since z˜ 2
    We explore the size evolution of 831 very massive galaxies (Mstar≥1011 h70-2 Msun) since z˜ 2 using the combined capabilities of the large near infrared Palomar...
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    Structural algorithms to solve radiative transfer problems
    Not Available
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    Structural analysis for the EST preliminary design specifications
    This contribution presents the structural analysis that followed the preliminary design specifications of the European Solar Telescope (EST). EST is a 4-metre...
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    Structural and thermal analysis of EMIR
    This paper shows the different design concepts and techniques employed in the structural and thermal analysis of EMIR (Espectrografo Multiobjeto Infrarrojo)...
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    Structural Components of NGC 5850
    Not Available
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    Structural properties of disk galaxies. I. The intrinsic equatorial ellipticity of bulges.
    A variety of formation scenarios have been proposed to explain the diversity of properties observed in bulges. Studying their intrinsic shape can help to...
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    Structure and components of an LTE stellar atmosphere model
    We summarize in this paper the principles for the algorithmic representation of the structure of a stellar atmosphere. The physical analysis of the problem...
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    Structure and dynamics of massive galaxies at z=0 in a fully cosmological simulation
    In this contribution we present the results of an Eulerian adaptive mesh refinement (AMR) hydrodynamical and N-body simulation in a ΛCDM cosmology. The...