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  • RGB image of the Ring Nebula obtained with WEAVE/LIFU
    Press release
    The William Herschel telescope at the Roque de los Muchachos Observatory discovers a mysterious iron “bar” in the Ring Nebula
    Research carried out with the new WEAVE spectrograph, installed on the William Herschel Telescope (WHT) at the Roque de los Muchachos Observatory (La Palma), and in whose construction the Instituto de Astrofísica de Canarias (IAC) has participated, has found a mysterious bar-shaped cloud of iron inside the iconic Ring Nebula. The study was conducted by a European team led by astronomers at University College London (UCL) and Cardiff University, and includes researchers from the IAC. The cloud of iron atoms, described for the first time in Monthly Notices of the Royal Astronomical Society
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  • Arianna Di Cintio, a researcher at the IAC and lecturer at the ULL, alongside José Oñorbe from Seville, a researcher and lecturer at the University, during the symposium ‘Computational Galaxy Formation & Large-Scale Structures’
    Press release
    The IAC is organising the SEA’s first symposium dedicated to the computational study of galaxy formation
    Arianna Di Cintio, a researcher at the Instituto de Astrofísica de Canarias and a lecturer at the University of La Laguna, chaired the organisation of this event, which took place as part of the 17th Scientific Meeting of the Spanish Astronomical Society (SEA). The symposium attracted more than 75 participants at each of its four sessions, featured over 30 scientific presentations and welcomed six guest experts. The Instituto de Astrofísica de Canarias (IAC) has organised the first symposium of the Spanish Astronomical Society (SEA) dedicated to the computational modelling of galaxies and
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  • Artistic impression of a runaway star propelled by a supernova explosion
    Press release
    IAC researchers participate in the largest Milky Way study of massive runaway stars
    Researchers from the Instituto de Astrofísica de Canarias (IAC), in collaboration with the Instituto de Ciencias del Cosmos de la Universidad de Barcelona (ICCUB) and the Instituto de Estudios Espaciales de Cataluña (IEEC), have carried out the largest observational study to date on massive runaway stars including rotation and binarity in the Milky Way. This work, recently published in Astronomy & Astrophysics , sheds light on how these stellar “fugitives” are launched into space and what their properties reveal about their intriguing origins. Runaway stars are stars that travel through
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