ESO

Artist's concept of a luminous blue variable star (ESO/L. Calçada)

An article published in the “Monthly Notices of the Royal Astronomical Society” reports the mysterious disappearance of a massive star of the luminous blue variable type in the Kinman dwarf galaxy. A team of researchers led by Andrew Allan of Trinity College in Dublin, Ireland, detected the disappearance of that star using ESO’s Very Large Telescope (VLT) in Chile. Additional observations and research of archival data to try to better understand the events led to believe that the most likely possibilities are a transformation that led to a sharp drop in brightness, maybe dimmed even more due to the dust that covered it, and its direct collapse into a black hole without a supernova explosion.

Artistic representation of an extreme horizontal branch star with a giant star spot

An article published in the journal “Nature Astronomy” reports a study on stars of a particular type since they’re much smaller than the Sun but much hotter and therefore blue. A team of researchers led by Yazan Al Momany of the Italian National Institute of Astrophysics, Padua, used various instruments on ESO’s Very Large Telescope (VLT) and NTT (New Technology Telescope) in Chile to study stars of that type discovering the equivalent of sunspots but even three thousand times larger in size. In some of these spots, flares have been observed that are millions of times more intense than the Sun’s which indicate the presence of very intense magnetic fields.

Artist's concept of the HR 6819 system

An article published in the journal “Astronomy & Astrophysics” reports the discovery of a black hole in a triple system known as HR 6819. A team of researchers led by ESO’s Thomas Rivinius used the FEROS spectrograph on the MPG/ESO 2.2 meter telescope at La Silla to examine that system in a study on binary systems, surprisingly discovering the presence of a third object identified as a black hole. It’s the closest black hole to the solar system, but according to the researchers it could be the tip of the iceberg, and there could be many others like that, as predicted by theoretical models.

Artist's concept of iron rain on the exoplanet WASP-76b (Image ESO/M. Kornmesser)

An article published in the journal “Nature” reports a study on the conditions existing on the exoplanet WASP-76b, an ultra-hot Jupiter where on the side illuminated by its star it’s so hot that metals vaporize and then condense on the dark side, where it rains iron. A team of researchers led by David Ehrenreich of the University of Geneva, Switzerland, used the ESPRESSO instrument mounted on the VLT in Chile to study the processes underway in the atmosphere of WASP-76b with the winds that carry the iron vapor across this gas giant.

NGC 2264 seen by Spitzer (Image Image Credit: NASA/JPL-Caltech/P.S. Teixeira (Center for Astrophysics))

NASA’s Spitzer space telescope captured a new image of the so-called Christmas Tree Cluster, so nicknamed for its shape. That appearance is enhanced by a remarkable star formation with the consequent presence of protostars that emit a light that appears pink or red to Spitzer that gives the area an effect similar to the Christmas tree’s balls. It’s part of a set of objects collectively known as NGC 2264 which also includes the Snowflake Cluster, the Cone Nebula and the Fox Fur Nebula.