Un estudio, realizado por un equipo de investigación del Instituto de Astrofísica de Canarias (IAC), revela que una inusual y delgada estructura de estrellas...
Evidence for the Accretion of Gas in Star-forming Galaxies: High N/O Abundances in Regions of Anomalously Low Metallicity
While all models for the evolution of galaxies require the accretion of gas to sustain their growth via on-going star formation, it has proven difficult to...
Physically Motivated Fit to Mass Surface Density Profiles Observed in Galaxies
Polytropes have gained renewed interest because they account for several seemingly disconnected observational properties of galaxies. Here we study whether...