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
The Instituto de Astrofísica de Canarias (IAC) has initiated a project of science outreach in the Tenerife-II prison in El Rosario, with the aim of bringing knowledge about the Universe to the prisoners, as well as to the educational and other working personnel at that centre. This initiative is taken in the framework of the commitment of the IAC to the popularization of science as a tool for inclusión and social transformation. The project is led by the astrophysicist, and IAC researcher David Aguado and is a continuation of a first experiment in 2024 in the Madrid V prison at Soto del Real
A study published today in Nature Astronomy , in which a researcher from the IAC has participated, outlines the discovery of an extremely rare type of binary system composed of two high mass white dwarfs. The two stars are so close together that they will eventually collide resulting in a supernova explosion which, due to its proximity to the Earth, will appear ten times brighter than the Moon. Type 1a supernovae are a class of cosmic explosion often used as "standard candles" to measure the expansion of the Universe. They occur when a white dwarf exceeds the Chandrasekhar mass - the limit
