Few days back a black hole, which had been dormant for 26 years, started showing signs of activity with x-ray and gamma ray bursts. NASA’s Swift satellite was the first to detect the rising tide of high-energy X-rays from the constellation Cygnus.
The outburst of x-rays and gamma rays came from V404 Cygni, a binary system located some 8,000 light-years away that contains a black hole. Every couple of decades the black hole fires up in an outburst of high-energy light, becoming an X-ray nova. Until the Swift detection, it had been slumbering since 1989.
In a matter of minutes after Swift detected the outburst, the Japanese experiment on the International Space Station called the Monitor of All-sky X-ray Image (MAXI) also picked up the flare. Then European Space Agency’s (ESA) Integral satellite also picked the outburst.
The term X-ray nova is used for a bright and short-lived X-ray source that reaches peak intensity in a few days and then fades out over a period of weeks or months. The outburst occurs when stored gas abruptly rushes toward a neutron star or black hole. By studying the patterns of the X-rays produced, astronomers can determine the kind of object at the heart of the eruption.
As these black hole eruptions are quite rare, one such a outburst is detected, scientists employ every possible satellite and experiments to analyse and monitor it says Neil Gehrels, Swift’s principal investigator at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.
The binary system like the V404 Cygni is classified as a low-mass X-ray binary wherein a star slightly smaller than the sun orbits a black hole 10 times its mass in only 6.5 days. The close orbit and strong gravity of the black hole produce tidal forces that pull a stream of gas from its partner. The gas travels to a storage disk around the black hole and heats up to millions of degrees, producing a steady stream of X-rays as it falls inward.
But the disk flips between two dramatically different conditions. In its cooler state, the gas resists inward flow and just collects in the outer part of the disk like water behind a dam. Inevitably the build-up of gas overwhelms the dam, and a tsunami of hot bright gas rushes toward the black hole.
Astronomers relish the opportunity to collect simultaneous multiwavelength data on black hole binaries, especially one as close as V404 Cygni. In 1938 and 1956, astronomers caught V404 Cygni undergoing outbursts in visible light. During its eruption in 1989, the system was observed by Ginga, an X-ray satellite operated by Japan, and instruments aboard Russia’s Mir space station.
“Right now, V404 Cygni shows exceptional variation at all wavelengths, offering us a rare chance to add to this unique data set,” said Eleonora Troja, a Swift team member at Goddard.
Ongoing or planned satellite observations of the outburst involve NASA’s Swift satellite, Chandra X-ray Observatory and Fermi Gamma-ray Space Telescope, as well as Japan’s MAXI, the European Space Agency’s INTEGRAL satellite, and the Italian Space Agency’s AGILE gamma-ray mission. Ground-based facilities following the eruption include the 10.4-meter Gran Telescopio Canarias operated by Spain in the Canary Islands, the University of Leicester’s 0.5-meter telescope in Oadby, U.K., the Nasu radio telescope at Waseda University in Japan, and amateur observatories.
V404 Cygni has flared many times since the eruption began, with activity ranging from minutes to hours. “It repeatedly becomes the brightest object in the X-ray sky — up to 50 times brighter than the Crab Nebula, which is normally one of the brightest sources,” said Erik Kuulkers, the INTEGRAL project scientist at ESA’s European Space Astronomy Centre in Madrid. “It is definitely a ‘once in a professional lifetime’ opportunity.”
In a single week, flares from V404 Cygni generated more than 70 “triggers” of the Gamma-ray Burst Monitor (GBM) aboard Fermi. This is more than five times the number of triggers seen from all objects in the sky in a typical week. The GBM triggers when it detects a gamma-ray flare, then it sends numerous emails containing increasingly refined information about the event to scientists on duty.
Every time the GBM recovered from one trigger, V404 Cygni set it off again, resulting in a torrent of emails. The event prompted David Yu, a GBM scientist at the Max Planck Institute of Extraterrestrial Physics in Garching, Germany, to comment on social media: “Achievement Unlocked: Mailbox spammed by a blackhole.”