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.

  • Artistic representation of the white dwarf star
    An international team of researchers led by the University of Warwick, with a member who is a scientist at the IAC has discovered white dwarf with unusual dimensions. This star could be, in fact, the result of the merger of two white dwarfs. The discovery is published today in the journal Nature Astronomy, and could resolve some questions about the evolution of white dwarfs, and about the number of supernova in our Galaxy. The star, which is 150 light years away, was identified by data from the satellite telescope GAIA of the European Space Agency (ESA). Based on these, the astronomers used
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  • Camera Drago
    A group of scientists and engineers from IACTEC Espacio, of the Instituto de Astrofísica de Canarias (IAC), will participate in the Second Spanish Small Satellites International Forum 2020 (SSIF) which will take place on 25th, 26th and 27th pf February in Málaga.The personnel from IACTEC-Espacio will present three studies on the development of technology which will help improve the working of nanosatellites as well as having a stand which will show off the developments and capacity of IACTEC. IACTEC (Space, Technology, Medicine and Large Telescopes) is the centre of technical and commercial
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  • José Miguel Rodríguez Espinosa
    At the next General Assembly of the International Astronomical Union (IAU), to be held in Korea in 2021, José Miguel Rodríguez Espinosa, a researcher at the Instituto de Astrofísica de Canarias will be named Secretary General of this, the biggest international astronomical organization, with over 13,500 professional astronomers in over 100 countries. For the time being he has been named Assistant General Secretary so that, afterwards, he will be able to take over the Secretariat. He will be the first Spaniard to occupy this position, which he will hold from 2021 to 2024. Rodríguez Espinosa
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  • Japanese delegation at the Roque de los Muchachos Observatory (La Palma)
    The Japanese ambassador to Spain, Kenji Kiramatsu, yesterday visited the Instituto de Astrofísica de Canarias (IAC) and the Canary Island Observatories, together with Masahiro Aoki, secretary to the Embassy, Yoshihiro Miwa, the consul of Japan in Las Palmas de Gran Canaria, and Josep Piqué Camps, President of the Council of the Spain Japan Foundation. Yesterday, they were received by Rafael Rebolo López, the Director of the IAC and Jesús Burgos, administrator of the General Services of the IAC at its headquarters in La Laguna. After a short visit, the delegation went up to the Teide
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  • Comparative Milky Way and ultra-diffuse galaxy
    A study by the Instituto de Astrofísica de Canarias (IAC), led by researchers Nushkia Chamba, Ignacio Trujillo and Johan H. Knapen, reveals that the enigmatic ultra-diffuse galaxies, very low-luminosity and low-density star galaxies, are similar in size to dwarf galaxies. The results, which are published in the journal Astronomy & Astrophysics, provide new clues about the number and type of galaxies in our Universe and about the nature of dark matter.
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  • A Milky Way-like spiral galaxy, a dwarf and a faint ultra-diffuse galaxy shown to the same physical scale using images of similar depth.  On average, the diffuse galaxy is 10 times smaller than the Milky Way analogue. Credit: Adapted from Chamba, Trujillo & Knapen (2020).
    Now almost 70 years since its introduction, the effective or half-light radius has become a very popular choice for characterising galaxy size. However, the effective radius measures the concentration of light within galaxies and thus does not capture our intuitive definition of size which is related to the edge or boundary of objects. For this reason, we aim to demonstrate the undesirable consequence of using the effective radius to draw conclusions about the nature of faint ultra-diffuse galaxies (UDGs) when compared to dwarfs and Milky Way-like galaxies. Instead of the effective radius
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