Líneas de investigación: La Vía Láctea y el Grupo Local (MWLG)
La Vía Láctea y el Grupo Local (MWLG)
Publicación
Stellar migration in the Auriga simulations
We study the presence and importance of stellar migration in the evolution of 17 Milky-Way like disc galaxies with stellar mass 10 < log(M */M ⊙) < 11 from the...
Stellar Wind Variations during the X-Ray High and Low States of Cygnus X-1
We present results from Hubble Space Telescope ultraviolet spectroscopy of the massive X-ray and black hole binary system, HD 226868 = Cyg X-1. The spectra were...
StraKLIP: A Novel Pipeline for Detection and Characterization of Close-in Faint Companions through the Karhunen-Loéve Image Processing Algorithm
We present a new pipeline developed to detect and characterize faint astronomical companions at small angular separation from the host star using sets of wide...
Strömgren Photometry of Galactic Globular Clusters. II. Metallicity Distribution of Red Giants in ω Centauri
We present new intermediate-band Strömgren photometry based on more than 300 u, v, b, y images of the Galactic globular cluster ω Cen. Optical data were...
Strong chemical tagging with APOGEE: 21 candidate star clusters that have dissolved across the Milky Way disc
Chemically tagging groups of stars born in the same birth cluster is a major goal of spectroscopic surveys. To investigate the feasibility of such strong...
Structure of the outer Galactic disc with Gaia DR2
Context. The structure of outer disc of our Galaxy is still not well described, and many features need to be better understood. The second Gaia data release...
Submillimetre galaxies reside in dark matter haloes with masses greater than 3×1011 solar masses
The extragalactic background light at far-infrared wavelengths comes from optically faint, dusty, star-forming galaxies in the Universe with star formation...
Surface abundances of CNO in Galactic O-stars: a pilot study with FASTWIND
Context. Rotational mixing is known to significantly affect the evolution of massive stars; however, we still lack a consensus regarding the various possible...