Left panel: map of the surface brightness of "the Antennae" in emission from ionized hydrogen. The brightest zones are the zones occupied by clusters of massive stars. Right panel: map of the expansion velocity of the bubbles detected in the Antennae, pus
Una delegación de la Universidad de La Laguna (ULL), encabezada por el rector Francisco García, ha realizado una visita institucional al Instituto de Astrofísica de Canarias (IAC), reforzando así el compromiso de colaboración y la estrecha relación que mantienen ambas instituciones, claves para el desarrollo científico y tecnológico de Canarias. El encuentro ha servido para revisar el estado del convenio que mantienen ambas instituciones y revisar algunas áreas de mejora para la renovación del mismo en materia de investigación, docencia y divulgación científica, además de aspectos
IAC researcher David Aguado has obtained a prestigious Starting Grant from the European Research Council (ERC), aimed at promoting promising young scientists. This is the third ERC grant -one of the most competitive and recognized of the Horizon Europe program- that the center has received so far this year, thus consolidating its international projection. These highly competitive grants provide up to €1.5 million over five years to support outstanding young scientists in establishing their own independent research groups and pursuing pioneering scientific ideas. Searching for the first stars
Massive stars in metal-poor galaxies often have close partners, just like the massive stars in our metal-rich Milky Way. This has been discovered by an international scientific team in which research staff from the Instituto de Aastrofísica de Canarias (IAC) and the Universidad de La Laguna (ULL) participate. They used the European Very Large Telescope in Chile to monitor the velocity of massive stars in the Small Magellanic Cloud. The research is published in Nature Astronomy . For the past twenty years, astronomers have known that many massive stars in the metal-rich Milky Way have a
