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An international collaboration, with the participation of the Instituto de Astrofísica de Canarias (IAC), determines with an unprecedented level of precision the mass, age and rotation profile of the core of a massive pulsating star. Known as HD 192575, it has been observed by the NASA space telescope TESS continuously for more than a year. The results shed new light on how such stars are internally structured and how they evolve until their death, when they explode as supernovae and form neutron stars and black holes. The scientific team has also used observations made with the MercatorAdvertised on
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The Deputy Director of the IAC, Casiana Muñoz Tuñón praises the bravery and persistence shown by Francisco Sánchez which enabled the IAC to be recognized as one of the best centres in the world for research in astrophysics. The Instituto de Astrofísica de Canarias (IAC) hosted this morning the ceremony to rename the Centre of Astrophysics on La Palma (CALP) as CALP Francisco Sánchez, in honour of the person who was the first Professor of astrophysics in Spain, and the founder of the IAC. Those taking part in the ceremony included the Founding Director of the IAC, Francisco Sánchez MartínezAdvertised on
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From 14 to 16 February, the second scientific meeting of the Laboratory for Innovation in Opto-Mechanics (LIOM) will be held at the IACTEC building managed by the Instituto de Astrofísica de Canarias (IAC) in the Science and Technology Park of La Laguna (Tenerife). This project is dedicated to the development of new optical and mechanical technologies that will form part of the next generation of telescopes capable of detecting biomarkers on exoplanets. One year after its creation, the IAC's Laboratory for Innovation in Opto-Mechanics (LIOM), is holding its second international meetingAdvertised on