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

An international team of researchers led by the Instituto de Astrofísica de Canarias (IAC) and the Universidad de La Laguna (ULL), has unveiled a breakthrough explanation for the origin of tiny, jet-like plasma ejections in the solar atmosphere, known as “nanojets.” These elusive events which are recently discovered by the NASA’s solar telescopes are thought to play an important role in heating and sustaining the solar corona at temperatures above one million Kelvin. Why Study Nanojets? For decades, solar physicists have been puzzled by the so-called “coronal heating problem.” While the Sun

On 12 August, to mark the total eclipse that will be visible across much of Spain, various towns in Palencia — including the capital, Frómista and Carrión de los Condes — will host a series of observation and outreach events bringing together scientists and students from Spain, Morocco and the United States. This event will serve as a training exercise for the NATE experiment, which will take place in North Africa during the next total eclipse next year, and will act as a meeting point between depopulated areas of Spain, the outermost regions, and Moroccan, American and Spanish students and