Astrofísicas: Nubes de Magallanes

  • Publicación
    A census of massive stars in NGC 346. Stellar parameters and rotational velocities
    Spectroscopy for 247 stars towards the young cluster NGC 346 in the Small Magellanic Cloud has been combined with that for 116 targets from the VLT-FLAMES...
  • Publicación
    A Detailed look at Chemical Abundances in Magellanic Cloud Planetary Nebulae. I. The Small Magellanic Cloud
    We present an analysis of elemental abundances of He, N, O, Ne, S, and Ar in Magellanic Cloud planetary nebulae (PNe) and focus initially on 14 PNe in the Small...
  • Publicación
    A stellar overdensity associated with the Small Magellanic Cloud
    We report the discovery of a stellar overdensity 8° north of the centre of the Small Magellanic Cloud (SMC; Small Magellanic Cloud Northern Over-Density; SMCNOD...
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    A study of the color-magnitude diagrams and luminosity functions of the two LMC clusters NGC 2134 and NGC 2249 with the new radiative opacities
    We present Johnson CCD photometry in the B and V passbands for the stellar content of two intermediate age star clusters of the Large Magellanic Cloud (LMC)...
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    Active star formation regions at the edge of the LMC Bar: NGC 1850 and NGC 1858
    We present UBV Johnson CCD photometry of two young clusters of the Large Magellanic Cloud (LMC), namely NGC 1850 and NGC 1858, which are located at the NW part...
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    Ages of LMC star clusters using ASAD2
    We use ASAD2, the new version of ASAD (Analyzer of Spectra for Age Determination), to obtain the age and reddening of 27 Large Magellanic Cloud (LMC) clusters...
  • Publicación
    Anomalous Cepheids in the Large Magellanic Cloud. Insight into their origin and connection with the star formation history
    Context. The properties of variable stars can give independent constraints on the star formation history of the host galaxy, by determining the age and...
  • Publicación
    Are extreme asymptotic giant branch stars post-common envelope binaries?
    Modelling dust formation in single stars evolving through the carbon-star stage of the asymptotic giant branch (AGB) reproduces well the mid-infrared colours...
  • Publicación
    Asymptotic giant branch stars in the Large Magellanic Cloud: evolution of dust in circumstellar envelopes
    We calculated theoretical evolutionary sequences of asymptotic giant branch (AGB) stars, including the formation and evolution of dust grains in their...
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