It may interest you
-
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 showAdvertised on -
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 delAdvertised on -
Research led by the Instituto de Astrofísica de Canarias (IAC) has discovered that, in binary systems, stars that evolve into red giants change the way they rotate with their companions, making their orbits more circular. The result was achieved after studying nearly 1000 solar-like oscillating stars in binary systems, the greatest yield to date of such objects. For their identification, the third Gaia Data Release (Gaia-DR3) and NASA Kepler and TESS catalogs have been explored. The study has been published in the journal Astronomy and Astrophysics and has been selected as the most recentAdvertised on