Left panel: map of the surface brightness of "the Antennae" in emission from ionized hydrogen. The brightest zones are the zones occupied by clusters of massive stars. Right panel: map of the expansion velocity of the bubbles detected in the Antennae, pus
En el marco del CXLVIII aniversario del nacimiento del ilustre científico canario Blas Cabrera y Felipe, la Real Sociedad Económica de Amigos del País de Tenerife (RSEAPT) acogerá una conferencia a cargo de Valentín Martínez Pillet, director del Instituto de Astrofísica de Canarias (IAC) y experto en Física Solar. La charla tendrá lugar el próximo martes 24 de febrero a las 18:00 horas en la sede de esta institución en La Laguna. Bajo el título “Viviendo con una estrella: el bueno, el feo y el malo”, Martínez Pillet explorará la relación entre la Tierra y el Sol. La charla, que forma parte
Researchers from around the world are taking part in the China–Spain Astronomical Collaboration on High-Resolution Spectroscopy 2025, an event organised by the Instituto de Astrofísica de Canarias (IAC) in collaboration with the National Astronomical Observatories of China (NAOC), the Nanjing Institute of Astronomical Optics & Technology (NIAOT), and the Gran Telescopio Canarias (GTC) team. The aim of the conference is to strengthen and consolidate scientific cooperation between China and Spain in the field of high-resolution spectroscopy, one of the key areas for studying stars, galaxies
Massive stars in metal-poor galaxies often have close partners, just like the massive stars in our metal-rich Milky Way. This has been discovered by an international scientific team in which research staff from the Instituto de Aastrofísica de Canarias (IAC) and the Universidad de La Laguna (ULL) participate. They used the European Very Large Telescope in Chile to monitor the velocity of massive stars in the Small Magellanic Cloud. The research is published in Nature Astronomy . For the past twenty years, astronomers have known that many massive stars in the metal-rich Milky Way have a
