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.

  •  Left panel: SINFONI data cube collapsed in the spectra dimension, where bot the interloper and Aql X-1 are clearly resolved. Right panel: averaged, normalized spectra obtained for each object.
    Low mass X-ray binaries consist of two components: a compact object (either a neutron star or a stellar-mass black hole) and a star with a mass similar or lower to that of the Sun. Both objects are close enough for the gravity to strip material from the companion star, which fall onto the compact object forming an accretion disc. Indeed, both objects are so close (typically less than three times the orbit of Mercury) that not even the most powerful telescope can spatially resolve them. Aquila X-1 (Aql X-1) is a canonical X-ray binary harbouring a neutron star. Since its discovery 40 years
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  • Strength of the large-scale magnetic field in nearby galaxies vs. their rotation speed.
    Magnetic fields are present on all scales in the Universe from planets and stars to galaxies and galaxy clusters, and even at high redshifts. They are important for the continuation of life on the Earth, the onset of star formation, the order of the interstellar medium, and the evolution of galaxies. Hence, understanding the Universe without understanding magnetic fields is impossible. The origin and evolution of cosmic magnetic fields is among the most pressing questions in modern astronomy. The most widely accepted theory to explain the magnetic fields on stars and planets is the α-Ω
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  • Oxygen and chlorine abundances in low-mass planetary nebulae (PNe) (black dots, from Delgado-Inglada et al. 2015) versus the new AGB model predictions for different masses (a few relevant masses are marked) and metallicities. The new models predict that O
    Recently, Delgado-Inglada and collaborators have shown that low-mass (between one and three times the mass of the Sun) planetary nebulae are rich in oxygen, but the standard theoretical models do not predict this. In this work we explain this phenomenon for the first time using theoretical models of nucleosynthesis (production of chemical elements in the interiors of stars) in their precursor AGB stars, which include convective processes, (which transport chemical elements created in the interior to the surface of the star) more efficient than in the standard models. This discovery calls
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  • Wide angle view from the Teide Observatory towards the east. Above the horizon you can see the planet Venus, an a little higher up and to the left of Venus is comet Catalina (C/2013 US10). The lights and villages are on Grand Canary. J.C. Casado-staryeart
    Several telescopes at the Teide Observatory (IAC) followed comet Catalina with the aim of characterizing its orbit dynamically. It should be possible to see the central zone of the comet with the naked eye, but to see details you would need binoculars.
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  • The 3.5m telescope on Calar Alto in Southern Spain. CARMENES is installed at this telescope, and will start searching for Earth-like planets orbiting nearby stars in early 2016.  Credits: Max-Planck-Institut für Astronomie
    CARMENES, an outstanding novel astronomical instrument, which has been designed to look for Earth-like planets, has successfully passed first “on-sky” tests at the telescope. Scientists and engineers of the Instituto de Astrofísica de Canarias (IAC) have participated in the design and construction of the new “planet hunter”.
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