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)
The PLATO (PLAnetary Transits and Oscillations of Stars) space mission, led by the European Space Agency (ESA), has recently completed one of the most delicate phases of its development: the integration of its main components, the 26 scientific cameras and the service module that houses all the instrument's acquisition, processing, and control electronics. This stage, carried out at the facilities of the aerospace company OHB in Germany, marks a fundamental step toward the launch scheduled for December 2026 from French Guiana aboard an Ariane 6 rocket. “Almost eight years after ESA gave the
La Fundación CajaCanarias organiza la octava edición de su Foro Enciende el Cosmos, que este año volverá a contar con la participación de destacados científicos e investigadores de reconocido nivel nacional e internacional. Esta iniciativa de carácter divulgativo pretende expandir, desde la exploración científica, la comprensión del Universo en su conjunto, relacionando el pasado con el presente y con una clara búsqueda de respuestas de cara al futuro. El programa se divide en tres sesiones, a celebrar los días 13 de febrero, 20 de marzo y 10 de abril, en el Espacio Cultural CajaCanarias de
The most massive stars in the universe are often born and evolve in binary and multiple systems — that is, in pairs or groups bound by their mutual gravity. Understanding how they interact with each other is key to explaining everything from their formation to the impact they have on the galaxies they inhabit. The MONOS project (Multiplicity Of Northern O-type Spectroscopic systems) aims to study these systems in the northern sky, combining spectroscopic observations (which analyze light split into its component colors to measure stellar velocities and physical properties) with photometry
