With the participation of the IAC, a total of 64,000 objects have been identified in the study of this region of massive star formation.
An international team of researchers, with participation from the Instituto de Astrofísica de Canarias, has discovered an extremely dense Neptune-sized planet, which challenges the conventional theories about the formation and evolution of planets. It was first identified with NASA’s TESS satellite, and the present studies were made with the HARPS-N spectrograph on the Telescopio Nazionale Galileo (TNG), at the Roque de los Muchachos Observatory (Garafía, La Palma, Canary Islands). The results of the study have been published in the journal Nature. It is called TOI-1853b and is really
La XXXIV Canary Islands Winter School of Astrophysics, organizada por el Instituto de Astrofísica de Canarias (IAC) y la Universidad de La Laguna (ULL), tendrá lugar entre los días 8 y 15 de noviembre. En esta edición, cerca de 60 estudiantes de 15 países se reunirán para conocer los últimos avances en el campo de la evolución de galaxias, con el Grupo Local como punto de referencia. Durante una semana, el edificio IACTEC, en el Parque Científico y Tecnológico de Tenerife (La Laguna), acogerá a 60 estudiantes de máster, doctorado y postdoctorado para nutrirse sobre las novedades del panorama
An international team of researchers, among them scientists from the Instituto de Astrofísica de Canarias (IAC), has confirmed the primitive origen of an old star in the Milky Way, using the ESPRESSO instrument. The stars with the least content of metals are considered to be the oldest in the Milky Way, formed only a few hundred million years after the Big Bang, which is a small fraction of the age of the universe. These stars are “living fossils” whose chemical composition gives clues about the first stages of the evolution of the universe. The star SMSS1605-1443 was discovered in 2018 and
