A team of astronomers led by ICE-CSIC analyzed for the first time a long radio-observation of a scallop-shell star in a pioneer study. The team observed the star using the Giant Metrewave Radio Telescope (GMRT) located in Pune (India), and related it to the photometric information from NASA’s Transiting Exoplanet Survey Satellite (TESS) and Las Cumbres Global Telescope Observatory. Scallop-shell stars are a recently discovered class of young M dwarfs. More than 70% of the stars in the Milky Way are M dwarfs, although there are only around 50 recently confirmed scallop-shell stars. They show

Dr. Rubén Sánchez-Janssen has been announced as the new Director of the Isaac Newton Group of Telescopes (ING). Dr. Rubén Sánchez-Janssen will follow in the footsteps of Dr. Marc Balcells. Dr Sánchez-Janssen is an Astronomer and Project Scientist at STFC’s UK Astronomy Technology Centre (UKATC), where he leads the development of scientific instrumentation and facilities for ground- and space-based astronomy from the ultraviolet to the near-infrared, with a particular emphasis on future missions. He specializes in galaxy evolution, with particular focus on low-mass galaxies and star cluster

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