Tipo de publicación: Sin árbitro

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    A novel technique to characterize the merging channel of the galaxies
    Most massive galaxies have grown their sizes during cosmic time. Several mechanisms have been proposed to explain this growth, being minor mergers the most...
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    A numerical laboratory for the diagnostics of stellar properties
    In a recent paper (Crivellari et al., 2003) we summarized the principles of the algorithmic representation of the structure of a stellar atmosphere. We...
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    A Numerical Study - of the Asymptotic Solutions to the Family C of the Periodic Orbits in the Restricted Problem of Three Bodies
    Not Available
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    A One Gyr Old Stellar Burst in NGC 6822?
    Not Available
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    A OSIRIS/GTC emission-line survey of the rich cluster Cl0024+2654 at z = 0.4
    In the framework of the GLACE project, we present the preliminary results of a mapping of emission lines (Hα+[NII], Hβ and [OIII]) in the rich cluster Cl0024...
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    A Parametric Model of the Solar Full-Disk Seismological Signal
    Solar eigenmodes frequencies are most often determined using some kind of modelisation of the Fourier spectrum of the data in one or two dimensions. Many...
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    A Period Distribution for M31 X-ray Transients from Chandra and HST
    All Galactic black hole binaries with low mass donor stars are transient X-ray sources; we expect most of the X-ray transients observed in external galaxies to...
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    A Photoionization Model of NGC 2363
    We present two selected photoionization models of the extragalactic H ii region NGC 2363, and compare them with three sets of observational data. We discuss the...
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    A Photometric and Magnetic Analysis of the Wilson Effect
    For two sunspot groups observed in June 1992 we analyze the center-to-limb variation and height dependence of various geometrical parameters describing the...