Líneas de investigación: La Vía Láctea y el Grupo Local (MWLG)

La Vía Láctea y el Grupo Local (MWLG)
  • Publicación
    Small-spatial-scale variations of nebular properties and the abundance discrepancy in three Galactic HII regions
    We present the results of long-slit spectroscopy in several slit positions that cover different morphological structures of the central parts of three bright...
  • Publicación
    SMASH: Survey of the MAgellanic Stellar History
    The Large and Small Magellanic Clouds are unique local laboratories for studying the formation and evolution of small galaxies in exquisite detail. The Survey...
  • Publicación
    SMASHing the LMC: A Tidally Induced Warp in the Outer LMC and a Large-scale Reddening Map
    We present a study of the three-dimensional (3D) structure of the Large Magellanic Cloud (LMC) using ∼2.2 million red clump (RC) stars selected from the Survey...
  • Publicación
    SMASHing the LMC: Mapping a Ring-like Stellar Overdensity in the LMC Disk
    We explore the stellar structure of the Large Magellanic Cloud (LMC) disk using data from the Survey of the MAgellanic Stellar History and the Dark Energy...
  • Publicación
    SMASHing the low surface brightness SMC
    The periphery of the Small Magellanic Cloud (SMC) can unlock important information regarding galaxy formation and evolution in interacting systems. Here, we...
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    Sodium-Oxygen Anticorrelation and Neutron-capture Elements in Omega Centauri Stellar Populations
    Omega Centauri is no longer the only globular cluster known to contain multiple stellar populations, yet it remains the most puzzling. Due to the extreme way in...
  • Publicación
    Solar Space Density of the Red Clump Stars and the Scale-Length of the Thin Disc
    We estimated the scale-length of the thin disc with the J and W1 magnitudes of the most probable red clump stars in the Galactic plane, - 0°.5 ⩽ b ⩽ +0°.5, in...
  • Publicación
    Solar-like oscillations in γ Cephei A as seen through SONG and TESS. A seismic study of γ Cephei A
    Context. Fundamental stellar parameters such as mass and radius are some of the most important building blocks in astronomy, both when it comes to understanding...
  • Publicación
    Solid state radiolysis of amino acids in an astrochemical perspective
    The aliphatic amino acids L-alanine and L-leucine and the aromatic amino acids L-phenylalanine, L-tyrosine and L-tryptophan were irradiated in the solid state...