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.

  • Diego Blas
    The gravitational force needed for the universe to evolve from when it was almost uniform, during the Big Bang, until galaxies, stars, and planets were formed is provided by the “dark matter”. But in spite of the essential role of this basic component, which is estimated to make up some 80% of the matter in the universe, scientists know virtually nothing about its nature, behaviour, and composition, which is one of the main challenges in current physics and cosmology. Aiming to give answers to these questions the researcher Diego Blas, Senior Lecturer in the Department of Physics of King’s
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  • ALMA cuásar
    Cristina Ramos Almeida, a researcher at the Instituto de Astrofísica de Canarias (IAC), has led research which used data from the ALMA telescope in Chile to understand how supermassive black holes impact the host galaxies they inhabit. The results are published today in the journal Astronomy & Astrophysics.
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  • Abell 370
    A team of researchers from the cosmology group at the Instituto de Astrofísica de Canarias has obtained one of the most accurate measurements of the masses of clusters of galaxies, and of their relation with the amount of hot gas in these clusters. To do this they have studied the dynamics of the galaxies in 570 clusters selected from the catalogue produced by the Planck satellite (ESA). This study has been produced during four years of work, in which over 10,000 spectra have been obtained with the Telescopio Nazionale Galileo (TNG) and the Gran Telescopio Canarias (GTC) at the Roque de los
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  • Norbert Langer
    Professor Norbert Langer is currently head of the Stellar Physics Group at the Argelander-Institut für Astronomie (Bonn, Germany). Considered one of the world’s leading experts in the field of theoretical stellar Astrophysics, for more than three decades he has been researching the evolution of high mass, from their early stages to the point when they explode as supernovae. These stars play an important role in the evolution of their host galaxies. However, their short lifetime makes them very difficult to observe, raising many questions about their nature. A correct interpretation of the
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  • Nebulosa y M31
    A recent study led by researchers at the Instituto de Astrofísica de Canarias (IAC) has resolved an old debate about the progenitor stars of the brightest planetary nebulae. The first author of this article, which has just been published in the journal Astronomy & Astrophysics, is Rebeca Galera Rosillo, a doctoral student at the IAC who passed away in 2020 when she was finishing this work for her doctoral thesis. The first and most important datum needed to grasp the nature of the universe is to know its size, to measure the distance to the galaxies. Just as in the Renaissance people began
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  • Left panel: spatial distribution of the auroral [N II] λ5755 emission line in the PN M 1-42 prior to applying the recombination contribution. Middle panel: spatial distribution of the N II λ5679 recombination line. Right panel: same as left panel after applying the recombination contribution correction.
    We present a detailed study of the gas chemical abundances in planetary nebulae (PNe), the final fate of solar-like stars, through high spatial resolution Integral Field Unit spectroscopy (IFU) obtained with the Multi Unit Spectroscopic Explorer (MUSE) attached to the 8.2-m Very Large Telescope (VLT) in Chile. We focused on three PNe with high abundance discrepancy factors (ADF > 20), which is a well-known and major unresolved problem in nebular astrophysics: chemical abundances obtained from faint optical recombination lines (ORL) yield systematically larger values than those obtained from
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