The first image of a new gaseous component in a planetary nebula.
False color image of the planetary nebula NGC 6778. In blue, the emission associated with weak lines of ion O++ recombination, taken with the OSIRIS tunable filter blue instrument in the GTC. In green, emission of the same ion in the excited lines by coll
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Jorge García Rojas: jogarcia_ext [at] iac.es (jogarcia_ext[at]iac[dot]es)
El Instituto de Astrofísica de Canarias (IAC), a través de su departamento IACTEC-Espacio, celebra hoy la System Requirements Review (SRR) de la misión IACSAT-1, un hito clave que marca la finalización de la fase B1 del proyecto y consolida todos los requisitos técnicos, científicos y programáticos necesarios para avanzar hacia el diseño preliminar del satélite. IACSAT-1 es la primera misión liderada íntegramente por el IAC dedicada a la observación astronómica desde el espacio. Se trata de un proyecto desarrollado por IACTEC-Espacio, con un equipo científico dirigido por el Prof. Rafael
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
An international team of researchers, including staff from the Instituto de Astrofísica de Canarias (IAC), has discovered a planetary nebula that destroyed its own planetary system, conserving the remaining fragments in the form of dust orbiting its central star. To date, more than 5000 exoplanets have been discovered orbiting stars of all kinds and almost every stage of stellar evolution. However, while exoplanets have been discovered around white dwarfs – the final stage in the evolution of low- and intermediate-mass stars like the Sun, no exoplanets have been detected in the previous