News
DEVELOPMENT OF HIGH SPATIAL RESOLUTION SYSTEMS.
Un instrumento cute-SCIDAR, desarrollado por el IAC, se ha probado recientemente (Nov 2007) con éxito en el Observatorio del Paranal. Este instrumento...
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NewsDevelopment of the IAC-STAR public programmeA public programme (IAC-STAR) has been developed for generating of HR and C-M synthetic diagrams to investigate problems of star formation and population...
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NewsDiffuse interstellar bands in proto-fullerene circumstellar environments.Fullerenes and fullerene-related molecules have been proposed as explanations for unidentified astronomical features such as the intense UV absorption band at...
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NewsDiscovered one of the brightest distant galaxies so far knownIn the phenomenon of gravitational lensing, predicted by Einstein's General Theory of Relativity, the mass of a galaxy acts on the light of a more distant...
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NewsDiscovery of a massive supercluster system at z=0.47Superclusters are the largest over-dense, relatively isolated systems in the cosmic web. They provide us invaluable information about the large-scale structure...
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NewsDiscovery of a massive black hole companion to a B-type star from radial velocity measurementsAll stellar-mass black holes have hitherto been identified by X-rays emitted from gas that is accreting onto the black hole from a companion star. These systems...
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NewsDiscovery of a young and massive stellar cluster: Spectrophotometric near-infrared study of Masgomas-1.Recent near-infrared data have contributed to the discovery of new (obscured) massive stellar clusters and massive stellar populations in previously known...
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NewsDiscovery of a young forming planet around the nearby star AU MicAU Microscopii (AU Mic) is the second closest pre-main-sequence star, at a distance of 9.79 parsecs and with an age of 22 million years . AU Mic possesses a...
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NewsDiscovery of a young planetary mass companion to the nearby M dwarf VHS J125601.92-125723.9In a search for common proper motion companions using the VISTA Hemisphere Survey (VHS) and the 2MASS catalogs we have identi fied a very red (J-Ks = 2.47 mag)...