Tipo de publicación: Sin árbitro

  • Publicación
    Study on the Abundance Discrepancy Problem in the Magellanic Clouds
    We present chemical abundances of carbon (C) and oxygen (O) in the Large and Small Magellanic Clouds from deep and high-quality optical spectra of H II regions...
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    Studying Barred Galaxies by Means of Numerical Simulations
    We describe two morphological structures of barred galaxies with the help of numerical simulations. The first one is a feature seen in face-on barred galaxies...
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    Studying galaxies at low and high redshifts with GRBs
    Not Available
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    Studying Galaxy Formation and Evolution from Local Group Galaxies
    In this contribution I present the main research activities of the IAC ``Stellar Populations in Galaxies'' research Group, with emphasis on the subtopics...
  • Publicación
    Studying Galaxy Formation and Evolution from Local Group Galaxies
    We present the main research activities of the IAC research Group ``Stellar Populations in Galaxies'', with emphasis on the topics that are directly related to...
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    Studying old populations with RR Lyrae Variables in the Local Group
    We want to study the characteristics and the physical extent of the old populations in a sample of Local Group galaxies in different environments, from the dSph...
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    Studying the Relationship Between the Average Velocity of the Turbulence and High Altitude Winds at the Teide Observatory
    The requirements for excellent image quality of current large and future very large telescopes demand a proper knowledge of atmospheric turbulence. Thus several...
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    Studying the Roots of the Supergalactic Wind in NGC 1569 with Gemini GMOS/IFUV
    We present Gemini North GMOS/IFU observations of the roots of the NGC 1569 super-galactic wind. This forms part of a larger and on-going study of the formation...
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    Studying the variability of the surface brightness of the Earthshine
    Lunar photometric observations are regularly taken from Big Bear Solar Observatory. The aim of these observations is to obtain the brightness ratio between the...