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)
A greedy white dwarf star in our own Milky Way galaxy is devouring its closest celestial companion at a rate never seen before, according to an international study involving the Instituto de Astrofisica de Canarias (IAC) and the University of La Laguna (ULL). The research, published in the journal Monthly Notices of the Royal Astronomical Society , found the double star, named V Sagittae, is burning unusually bright as the super-dense white dwarf is gorging on its larger twin in a feeding frenzy. Experts think the stars are locked in an "extraterrestrial tango" as they orbit each other every
El Cherenkov Telescope Array Observatory (CTAO) , el futuro observatorio de astronomía de rayos gamma más grande y potente del mundo, continúa su avance constante hacia su fase de operaciones iniciales. En una rueda de prensa conjunta celebrada en Santa Cruz de La Palma, Islas Canarias (España), representantes de la Organización Central del CTAO (CTAO ERIC), la Colaboración LST del CTAO , el Cabildo de La Palma y el Instituto de Astrofísica de Canarias (IAC) se reunieron para destacar el avance del proyecto hacia una ciencia pionera. Este progreso está marcado por la próxima inauguración de
An international scientific team, including members of the Instituto de Astrofísica de Canarias (IAC), has launched an ambitious program to map exoplanets located around the Neptunian Desert —a region around stars where planets the size of Neptune are very rare— in order to better understand the mechanisms of planetary system evolution and formation. This scientific expedition has delivered its first results with the observation of the TOI-421 planetary system. Analysis of this system reveals a surprisingly inclined orbital architecture, offering new insights into the chaotic history of