An article published in the journal “Nature” describes a research that shows a new function of the “tentacles” of the so-called jellyfish galaxies. An international team of astronomers led by Bianca Poggianti of the INAF-Astronomical Observatory of Padua in Italy used the observations conducted during ESO’s GASP program with the MUSE instrument installed on the Very Large Telescope (VLT), discovering that the mechanism that generates those tentacles is the same that powers the supermassive black holes at the center of those galaxies.
Blogs about black holes
An article published in “The Astrophysical Journal” describes an analysis of the motions of stars that orbit the supermassive black hole at the center of the Milky Way, particularly the one known as S2. A team of astronomers applied a new analytical technique to observations conducted in the past with ESO’s Very Large Telescope (VLT) in Chile and other telescopes concluding that those orbits are influenced by the effects of Albert Einstein’s theory of general relativity.
An article published in the journal “Astronomy & Astrophysics” describes a research involving 16 of the brightest known quasars. A team of researchers led by the Italian National Institute of Astrophysics (INAF) examined in particular those quasars’ infrared emissions to identify young hot stars in the galaxies hosting them concluding that a lot of them are forming, at a rate up to about 4,000 times higher than in the Milky Way.
An article published in “The Astrophysical Journal” describes a research suggesting that in primeval galaxies of the type called dusty starburst – because dust filters their light – star formation activity can be inhibited by the presence of a quasar. A team of astronomers from Iowa University used the ALMA radio telescope to locate the quasars and then other telescopes to observe them at various wavelengths.
An article published in the journal “Nature” describes the observation of a gamma-ray burst named GRB 160625B. An international team of astronomers led by Eleonora Troja of the University of Maryland used a number of telescopes after its discovery with NASA’s Fermi space telescope to detect the properties of this extremely energetic event, its geometry, the orientation of its jets and the origin of its extremely bright optical flash.