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)
An international team composed of Drs. Sylvain G. Korzennik, from the Center for Astrophysics | Harvard & Smithsonian , and Antonio Eff-Darwich Peña, from the University of La Laguna and the Instituto de Astrofísica de Canarias, has published a pioneering study aimed at improving our understanding of the Sun’s internal structure. The work, published in The Astrophysical Journal , stands out for its use of exceptionally long helioseismic time series, exceeding twenty-five years of continuous observations, to analyze the deepest layers of the Sun. Helioseismology is the study of patterns of
The European Solar Telescope (EST) has successfully completed the Conceptual Design Review (CoDR) of its Scientific Instrument Suite (SIS). The scientific objectives of EST focus on examining magnetic coupling in the solar atmosphere from the deepest layers of the photosphere to the highest layers of the chromosphere. This will enable the thermal, dynamic and magnetic properties of solar plasma to be studied with high spatial and temporal resolution. These objectives are defined by the Science Advisory Group (SAG), an international group of experts responsible for establishing the scientific
