X-rays emitted from the black hole flicker following a pattern that lasts for a few months and then suddenly ends. The phenomenon is predicted by Einstein’s general relativity and now astronomers were able to measure it in such strong gravitational fields.

One of the main goals of the AHEAD project is to offer the possibility for scientists and PhD students in astronomy to visit major astrophysical institutes and data centers and perform data analysis by accessing data archives and software tools, Read More …

Astronomers observed a binary star system that contains a low-mass star and a black hole. The black hole pulls material from its companion star extremely slowly and therefore emits only a very small amount of X-rays. “It is so quiet that it is practically a stealth black hole”.

Astronomers caught a supermassive black hole consuming a star that was drifting in space. The star was eaten so fast by the black hole that the Eddington limit –the theoretical maximum speed limit that defines how fast matter can be consumed by a black hole, was briefly exceeded.

Since the discovery of the Van Allen radiation belts, about 50 years ago, a complete explanation of their dynamics remains elusive. Now, astronomers have developed a new theoretical model than offers a plausible explanation for their formation.

The accretion disk that surrounds black holes emits X-rays that often show rhythmic pulses. These are known as quasi-periodic oscillations (QPOs) and their exact nature remains unknown.

Magnetars are the strongest magnets in the universe. 29 magnetars have been detected to date, but the exact physical mechanism(s) that creates them remains unknown. Recently, astronomers, discovered another unusual feature in one of these magnetars; a wind nebulae.

Astronomers know that supermassive black holes that live in the centre of massive galaxies are fed by hot ionized gas from the galaxy’s halo. Recent observations reveal that chaotic, cold rain is also included in their diet.

An outstanding question in modern astronomy is how can growing black holes be so critical in the formation and evolution of their host galaxy when they are billion times more compact than the galaxies in which they reside in? KMOS, an instrument operating at VLT will allow scientists to answer this question and more.

Astronomers developed a new theory for the formation of supermassive black holes. Data from NASA’s Great Observatories support their theoretical framework.

The X-ray XMM-Newton space telescope in October 12th, 2021 completed its 4000th orbit around the Earth with a billion kilometers travelled so far! XMM-Newton is an European Space Agency X-ray satellite launched in December 10th of 1999. The mission was Read More …

Astronomers have measured motions within a remarkable cosmic structure for the first time using NASA’s Chandra X-ray Observatory. The data show a blast wave and debris from an exploded star moving away from the explosion site and colliding with a Read More …

Astrophysicists have used computer simulations to show that in deep in space, tsunami-like structures may form on much bigger scales than here on Earth, from gas escaping the gravitational pull of a supermassive black hole. In fact, the mysterious environment Read More …

Published on Nature Communications the work led by Samuele Ronchini, PhD student at GSSI and INFN associate, together with INAF, which sheds new light on cooling processes happening in jets of Gamma-Ray Bursts. What are the processes that determine the Read More …

After the discovery of quasars (QSO), in the mid-1960s the X-ray astronomy started and was important to understand better the nature and the properties of the Active Galactic Nuclei (AGN), as the X-ray emission seemed to occur in the majority Read More …

A new panorama from NASA’s Chandra X-ray Observatory and the MeerKAT radio telescope provides a stunning view of the center of our Milky Way galaxy. It also reveals threads of superheated gas and magnetic fields, which are weaving a tapestry Read More …

The Athena (Advanced Telescope for High ENergy Astrophysics) mission is the second long-range space mission (L2) of the long term program “Cosmic Vision” of the European Space Agency (ESA). This mission is dedicated to the scientific theme “The hot and Read More …