El embajador de Japón en España, Takahiro Nakamae , visitó esta semana la sede central del Instituto de Astrofísica de Canarias (IAC) y el Observatorio del Teide, junto con Shinji Yamada, cónsul de Japón en Las Palmas de Gran Canaria, junto a personal de su equipo. En la sede central fueron recibidos por Valentín Martínez Pillet, director del IAC; y por el responsable de Instrumentación, Marcos Reyes; y por la jefa de la Unidad de Comunicación y Cultura Científica (UC3), Verónica Martín. En la sede central del IAC conocieron las instalaciones y las principales líneas de investigación del

An international piece of research, led by the Instituto de Astrofísica de Canarias (IAC) has found clues to the nature of some of the brightest and hottest stars in our Universe, called blue supergiants. Although these stars are commonly observed, their origin has been an old puzzle that has been debated for several decades. By simulating novel stellar models and analysing a large data sample in the Large Magellanic Cloud, IAC researchers have found strong evidence that most blue supergiants may have formed from the merger of two stars bound in a binary system. The study is published in the

A study led by researcher Laura Scholz, of the Instituto de Astrofísica de Canarias (IAC) has found, for the first time, observational evidence that the evolution and the properties of the galaxies are conditioned not only by the mass of the stars they contain, but aso by the effect of the dark matter halos which surround them. The results are published in the specialist journal Nature Astronomy. Dark matter comprises around 85% of all the matter in the Universe. Although ordinary matter absorbs, reflects and emits light, dark matter cannot be seen directly, which makes its detection