News

This section includes scientific and technological news from the IAC and its Observatories, as well as press releases on scientific and technological results, astronomical events, educational projects, outreach activities and institutional events.

  • The stellar source for phosphorus, element so important for life, is still unknown. Credit: Gabriel Pérez Díaz, SMM (IAC).
    All chemical elements in the Universe (except for H and most of the He) have been made in stellar interiors. But among those elements, the ones that allowed to build life such as we find on Earth are of particular interest (carbon, nitrogen, oxygen, sulphur and phosphorus). However, the stellar origin of phosphorus (P) is still unknown as none of the current models of Galactic chemical evolution can explain all the phosphorus we observe in the Galaxy and notably in our Solar System, highlighting a still lacking phosphorus source. In this work we report the discovery of stars very rich in
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  • Scheme which represents the origin of phosphorus on Earth, with respect to possible stellar sources of phosphorus in our Galaxy. Credit: Gabriel Pérez Díaz, SMM (IAC).
    The journal Nature Communications today is publishing the discovery of a new type of stars, very rich in phosphorus, which could help to explain the origin of this chemical element in our Galaxy. This achievement has been made by astronomers of the Instituto de Astrofísica de Canarias (IAC) and researchers in computer science from the Centre for Research in Information and Communication Technology (CITIC) at the University of La Coruña (Galicia).
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  • Image illustrating the comparison between an active spiral galaxy (orange box) and its non-active twin (blue box). Credit: Gabriel Pérez Díaz, SMM (IAC).
    A study led by researchers at the Instituto de Astrofísica de Canarias (IAC), making comparison between the discs of several pairs of spiral galaxies, active and non-active, concludes that in the discs of the former the rotational motion of the stars is of greater importance. This study, just accepted for publication in Astronomy & Astrophysics Letters, is the first evidence for large scale dynamical differences between active and non-active galaxies in the local universe. The astronomers participating are from the Instituto de Astrofísica de Canarias (IAC) and the University of La Laguna
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  • Artist's impression of a star pulsating in one of its hemispheres due to the gravitational attraction of a companion star. Credit: Gabriel Pérez (SMM-IAC).
    It has long been suspected that tidal forces in close binary stars could modify the orientation of the pulsation axis of the constituent stars. Such stars have been searched for, but until now never detected. Here we report the discovery of tidally trapped pulsations in the ellipsoidal variable HD 74423 in Transiting Exoplanet Survey Satellite (TESS) space photometry data. The system contains a Delta Scuti pulsator in a 1.6 d orbit, whose pulsation mode amplitude is strongly modulated at the orbital frequency, which can be explained if the pulsations have a much larger amplitude in one
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  • Spitzer images of the galaxy M87. Credit: NASA/JPL-Caltech/IPAC/Event Horizon Telescope Collaboration
    A Master’s degree research project at the University of Barcelona (UB), carried out at the Instituto de Astrofísica de Canarias (IAC) by the student Alejandra Yrupe Fresco, currently studying for her doctorate at the Max Planck Institute for Extraterrestrial Physics, in Germany, has revealed the faint nucleus and the structure of the jet of particles in the nuclear region of M87, the brightest galaxy in the Virgo cluster. This project was carried out in collaboration with the IAC researchers Juan Antonio Fernández Ontiveros, Almudena Prieto and José Antonio Acosta Pulido, and was possible
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  • Frame of the video Traveling on a Comet. Credit: Virtualisrealitates
    To celebrate Asteroid Day, which commemorates the impact of the Tunguska Fireball in 1908, several researchers from the Instituto de Astrofísica de Canarias (IAC) will participate in on-line chats to talk about the nature of these lesser bodies of the Solar System, and about the risk of impact on the Earth.
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