The first image of a new gaseous component in a planetary nebula.
False color image of the planetary nebula NGC 6778. In blue, the emission associated with weak lines of ion O++ recombination, taken with the OSIRIS tunable filter blue instrument in the GTC. In green, emission of the same ion in the excited lines by coll
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Jorge García Rojas: jogarcia_ext [at] iac.es (jogarcia_ext[at]iac[dot]es)
The IAC's Educational Project with Robotic Telescopes (PETeR) offers a new edition of its online teacher training entitled ‘ Investigate the Universe with Robotic Telescopes’. This activity, organised in collaboration with the STEAM area of the regional Ministry of Education of the Canary Islands Government, aims to provide knowledge and tools to incorporate astronomy in the classroom through the use of professional robotic telescopes, the analysis of scientific data and active learning methodologies. PETeR is an educational project that gives schools free access to professional telescopes
The Instituto de Astrofísica de Canarias (IAC) today held the 16th edition of the ‘Our Science Day’, an annual internal event which brought together its research and technical staff at the IACTEC headquarters in La Laguna. This meeting has established itself as a space for sharing the most outstanding advances of the past year in the different areas of work of the centre, promoting collaboration, cohesion and the exchange of ideas between teams. The conference was opened by the director of the IAC, Valentín Martínez Pillet, who presented an analysis of the centre's situation. The director
O ne of the key challenges in astronomy is to measure accurate distances to celestial objects. Knowing distances is crucial since it allows us to measure physical properties such as size, mass and luminosity. Since we can’t go out and use a tape-measure, a range of different approaches have been developed. Many of these approaches rely on using “standard candles”. Standard candles are objects (for example stars or supernovae) for which we know their intrinsic ”true” brightness. Once we know this, then their observed brightness compared to their intrinsic brightness gives us a distance to the
