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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.

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  • RSG1 is an enormously massive cloud in the Milky Way.
    Research news
    Search for and analysis of IR clouds
    LIRIS, the IR imaging camera and spectrograph built by the IAC, is giving life to new projects. During 2006 advances were made in the search for and analysis of IR clouds. RSG1 is shown in Figure 1. It is a cloud with fourteen red supergiants, (indicated in the figure, together with the relative coordinates at the centre of the cloud), implying that the it has a mass of 2-4 x 104 M¤. This would make it one of the most massive clouds in the Milky Way. Figure II shows the cloud ID066. The centre of the cloud can be seen with an extinction zone around it, which could have come from the original
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  • Composite image of the Orion Nebula in the [NII], Ha and [OIII] emission lines, codified respectively in red, green and blue. The details in black and white, to the side, illustrate the fields of motion divided into two zones of the nebula during the extr
    Research news
    Variability in the Orion nebula
    Using images from the HST archive of the Ha and [OIII] l5007A emission lines that are 6.84 years apart, variability in the temperature and density of ionized gas has been detected in intervals of one hundredth of a pc. The temperature variations are in the order of tens of degrees centigrade. Possible mechanisms for explaining this variability have been put forward, including the reconnection of magnetic fields induced by supersonic turbulence in the HII region. At the same time, it has been possible to detect and map the field of motion of gas driven by young or forming stellar winds
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  • Light curves of TRES_2 obtained using telescopes of the network and with two telescopes from the Observatorio del Teide: "IAC-80" and "TELAST" with different filters.
    Research news
    TrES-2
    In August 2006 a new planetary transit was discovered from data from the TrES network. The discovery was confirmed using radial velocity curves obtained with the Keck and characterised with light curves in different filters obtained using two telescopes at the Observatorio del Teide: "IAC80" and "TELAST" (the first result of scientific interest obtained from the latter). The planet discovered, TrES-2, is more massive and somewhat larger than its quasi-homonym TrES-1 (the first exoplanet discovered using the transit method), and follows the expected patterns for this type of object. Its main
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