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The distribution of planets in the over five thousand distant solar systems discovered to date forms a complex puzzle. There is a region in the planetary orbit graph, known as the " Neptunian desert", where very few Neptune-like planets with orbits of between two and four days period around their star have been recorded to date. Now, a scientific team led by the Instituto de Astrofísica de Canarias (IAC) and the Instituto de Astrofísica de Andalucía-Consejo Superior de Investigaciones Científicas (IAA-CSIC) , using a novel technique, new planets around red dwarf stars located precisely inAdvertised on
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This week, the Instituto de Astrofísica de Canarias is hosting the Second SONG Scientific Congress to conclude the first decade of high-level work of this international network devoted to the study of the interior of stars and the planetary systems that surround them. The meeting, which is taking place at the headquarters of IACTEC in La Laguna from 18 to 20 September, brings together more than 50 scientists from Europe, the United States, Australia and China to discuss the latest state-of-the-art techniques in time-resolved spectroscopy and stellar astrophysics. The Stellar ObservationsAdvertised on
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An international study led by Almudena Prieto, a researcher at the Instituto de Astrofísica de Canarias (IAC) has found places where new stars are forming, as faint star clusters, around the centre of an evolved galaxy. This is the first time that young populations of stars have been picked out and dated in this type of galaxies dominated by very old stars, which can be called “rejuvenated old galaxies”. The research has combined observations from various telescopes, both ground based and space based, and has used innovative techniques of data analysis. The results are published in theAdvertised on