Severo Ochoa Programme

Research News

  • Imagen artística de las primeras supernovas de la Vía Láctea. La estrella Pristine 221.8781+9.7844 se formó a partir del material eyectado por estas primeras supernovas. Crédito: Gabriel Pérez, SMM (IAC).
    An international team of researchers, including David S. Aguado, Jonay González and Carlos Allende Prieto of the Instituto de Astrofísica de Canarias (IAC), has found a star with extremely low metallicyt, one of the oldest in the Milky Way, and for that reason an excellent messenger from the early universe.
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  • This artist's rendering shows a disk of dust and planetary fragments around a star. Credit: NASA/JPL-Caltech. 
    The study, led by Paula Izquierdo, a doctoral student at the Instituto de Astrofísica de Canarias (IAC) and the University of La Laguna (ULL), has gone deeply into the analysis of this exceptional white dwarf, which shows periodic transits produced by fragments of a shredded planetesimal. The observations used for this research were obtained with the Gran Telescopio Canarias and with the Liverpool Telescope.
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  • Kepler's Supernova remnant. Crédito: X-ray: NASA/CXC/NCSU/M.Burkey et al; Optical: DSS. Release date: March 18, 2013.
    A study involving a researcher from the Instituto de Astrofísica de Canarias (IAC), which has been led by a researcher at the Instituto de Física Fundamental (IFF-CSIC) and the Instituto de Ciencias del Cosmos (UB-IEEC), argues that the explosion that Johannes Kepler observed in 1604 was caused by a merger of two stellar residues.
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  • Image of the Sun from GONG telescopes network in Hα filter. Prominences are seen as dark filaments over the solar disk. The arrow indicates a prominence that oscillates. The diagram shows the horizontal velocity of the prominence. In the first phase of th
    An international team led by researchers from the Instituto de Astrofísica de Canarias (IAC) and the Universidad de La Laguna (ULL) has cataloged around 200 oscillations of the solar prominences during the first half of 2014. Its development has been possible thanks to the GONG network of telescopes, of which one of them is located in the Teide Observatory.
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