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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.

List view
  • Background is a Hubble Space Telescope image of the relic galaxy, NGC 1277 (Credits: NASA, ESA, M. Beasley, and P. Kehusmaa). Bottom-left shows the H-band spectrum of the relic galaxy, NGC 1277, obtained with the EMIR spectrograph (middle) at Gran Telescopio Canarias (left) (Credits: pictures of GTC and EMIR are from GTC website).
    Research news
    New insights into the puzzle of strong CO absorptions in massive early-type galaxies

    Puzzling properties of massive early-type galaxies (ETGs) emerge when studying their spectra at near-infrared (NIR) wavelengths. Massive ETGs show strong CO absorption features in their H and K band spectra that cannot be explained by state-of-the-art stellar population models. For many years, the disagreement has been attributed to the presence of intermediate-age (0.1-2 Gyr) stellar populations in these galaxies, as the NIR light of intermediate-age stellar populations is dominated by cool stars (e.g. asymptotic giant branch (AGB) stars) that show strong CO absorptions in their spectrum

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  • Images of the article
    Press release
    Magnetic Fields in the Solar Atmosphere

    The prestigious journal Annual Review of Astronomy and Astrophysics invites two researchers from the Instituto de Astrofísica de Canarias (IAC) to publish an article reviewing the most important advances in the study of the magnetic fields in the outer regions of the solar atmosphere. Every year, the editorial committee of the journal Annual Review of Astronomy and Astrophysics (ARAA) meets to decide which researchers to invite to prepare their reviews, one for each field in Astrophysics. One of the 12 articles of the recently published volume 60 has been written by the IAC researchers

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  • Sextans A
    Press release
    The first extensive catalogue of massive stars with low metallicity

    A recent study, led by the Centre for Astrobiology (CAB, CSIC-INTA) with participation by the Instituto de Astrofísica de Canarias (IAC) presents the first extensive sample of massive stars whose chemical composition shows a lower metal content than that of the Small Magellanic Cloud. This is a basic first step in performing an exhaustive characterization of the properties of massive stars with low metallicity. Massive stars with very low metallicity are important for interpreting the processes which took place in the early phases of the univers, such as reionization and early chemical

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  • Artistic impression of the BL Lac nucleus. The particle jet emerging from the black-hole follows the spiral structure of the magnetic field. In the inset the brightness variations are shown as observed in red light (2020, August).
    Research news
    Rapid quasi-periodic oscillations in a relativistic jet

    Active galactic nuclei (AGN) consist of a supermassive black hole fed by the circumnuclear material close to the galaxy center. Around 10% of the AGNs develop a pair of jets that are launched to the interstellar medium at speed close to velocity of light. Blazars are observed when one of the jets points very close to our line of sight, which produce an extraordinary boosting of the emission by relativistic effects. Jets produce electromagnetic emission that varies rapidly and covers from radio waves to gamma rays. The observed light is mostly random without an apparent pattern. The source BL

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  • CLASP2.1
    Press release
    The CLASP2.1 mission team receives a NASA award

    The international team of the “Chromospheric LAyer Spectro-Polarimeter” (CLASP) space missions, which includes three scientists of the Instituto de Astrofísica de Canarias (IAC), has just received the NASA Group Achievement Honor Award for the successful execution of the recent CLASP2.1 mission. The goal of this mission is to map the magnetic field of the Sun in an extended region of the chromosphere. The Chromospheric Layer Spectro-Polarimeter series of heliophysics sounding rocket missions were designed to measure the polarization of the ultraviolet light emitted by the Sun to study the

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  • Errant intermediate-mass black holes
    Press release
    The possible detection of elusive intermediate mass black holes

    A research team at the Instituto de Astrofísica de Canarias (IAC) has observed an unusual type of emission in a sample of local galaxies which could indicate the presence of accretion discs around intermediate mass black holes (IMBH). The discovery would multiply by five the numer of known IMBH and opens a new way to detect and study this mysterious class of astronomica objects. Although only a few are known, via indirect evidence, the IMBH are a key to understand the formation of supermassive black holes and the galaxies which harbour them. The IMBH is a type of black hole whose mass is

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