ScienceNot yet confirmed elsewhere1 publisher2 min readPublished
Astronomers tie a 10-minute X-ray flash seen by Einstein Probe to merging neutron stars
Astronomers attribute EP250704a, a half-second gamma-ray burst followed by 10 minutes of X-rays, to two neutron stars colliding. The event gives them a test case for the hundreds of X-ray flashes Einstein Probe has logged since its 2024 launch, some of them still unexplained.
The Scientist · Science desk

What happened
- Einstein Probe, a joint European-Chinese mission, saw the blast on July 4, 2025, and its alert sent a team to ESO's Very Large Telescope, the Very Large Array and other telescopes.
- Niccolò Passaleva, who led the VLT observations, called it "the longest-lasting prompt X-ray flash ever observed from a neutron star merger."
- The researchers ruled out a supernova as the cause and found that the light had been travelling to Earth for 6 billion years.
- The team's results were published in the journal Science Bulletin.
Why it matters
- capability If minutes-long X-ray emission can mark a neutron-star merger, wide-field X-ray surveys gain a second way to spot mergers besides the gamma-ray flash that fades within two seconds.
- decision Teams following up Einstein Probe's unexplained flashes now have a merger origin to test against each one, alongside the supernova explanation.
- precedent Each further flash classified this way adds to a sample that, according to Passaleva, could show how often neutron-star mergers produce magnetars.
The X-ray emission lasted about 1,200 times as long as the gamma-ray spike before it [16]. Neutron-star mergers, the collisions space.com credits with forging gold, silver and platinum [12], have long been associated with gamma-ray flashes that fade within two seconds [5]. Some new research suggests that mergers can also show up as X-ray blasts lasting minutes [6].
The long X-rays caught the team's attention early. "When I saw the X-ray data from this new event, I realized something was up," said Eleonora Troja, a member of the Einstein Probe European collaboration [15]. The team's explanation for the extra minutes is a magnetar. According to space.com, the researchers think at least one was involved in the merger [9].
A collapsing stellar core can spin the neutron star it leaves behind up to more than 700 rotations a second [13]. The collapse also squeezes the magnetic field lines together, which strengthens the field. A core that starts out strongly magnetised can end as a magnetar, the object with the strongest magnetic field in the universe [13]. Troja framed the idea as a conditional. "If the remnant of the collision is a magnetar, it could keep bursting for longer," she said. "Magnetars are rapidly spinning neutron stars with huge magnetic fields. When they dump their magnetic power into the surroundings, they can make any explosion brighter and longer-lasting." [10]
We treat the merger as the team's best current interpretation. In space.com's account, the case rests on ruling out a supernova [8]. The account does not describe any positive sign of a merger in the VLT or VLA data, such as the kilonova light that marks these collisions [5].
Then there is the denominator. Since it launched in 2024, Einstein Probe has recorded hundreds of X-ray flashes in distant galaxies, and some have defied explanation [7]. EP250704a is one of them, a single event set against a count in the hundreds. It also came with a half-second gamma-ray burst [1]. On its own, then, it cannot show that an X-ray survey finds mergers a gamma-ray instrument would miss. If the merger reading holds, it does show that a merger can keep producing X-rays for 10 minutes [1].
What to watch
- An Einstein Probe flash with no gamma-ray counterpart that follow-up observations tie to a merger, the case needed to show X-ray surveys find mergers gamma-ray triggers miss.
- Whether other groups working from the VLT and VLA data reach the same merger interpretation, and whether any kilonova light is reported.
Clarity's read
What the record supports and how the coverage leans. The claims behind it follow.
Reality
- Evidence45
- Adoption
- Insufficient
- Hype gap+10
- Incentives
- Insufficient
- Confidence40
Claim ledger
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- [1]
EP250704a was first seen on July 4, 2025, as a blast of gamma rays lasting half a second followed by a bright X-ray emission lasting 10 minutes.
- [2]
The joint European-Chinese Einstein Probe witnessed the July 4, 2025 blast; after its alert, a team of astronomers studied the aftermath using ESO's Very Large Telescope, the Very Large Array and other telescopes.
- [3]
"This is the longest-lasting prompt X-ray flash ever observed from a neutron star merger," said Niccolò Passaleva, who led the observations of the X-ray flash with the VLT.
- [4]
The astronomers believe EP250704a may have come from a collision between two neutron stars.
- [5]
Neutron star mergers, marked by flashes of light called kilonovas, have long been associated with flashes of high-energy gamma rays that disappear within two seconds.
- [6]
New research suggests some neutron star mergers could reveal themselves via blasts of X-rays lasting minutes.
- [7]
Einstein Probe has discovered hundreds of X-ray flashes in distant galaxies since its launch in 2024; some have been linked to supernova deaths of massive stars, others have defied explanation, and EP250704a is one of the unexplained ones.
- [8]
The researchers ruled out a supernova as the cause of the X-ray burst and determined that the light from the collision has been travelling to Earth for 6 billion years.
- [9]
The team thinks the neutron star merger involved at least one magnetar.
- [10]
"If the remnant of the collision is a magnetar, it could keep bursting for longer," Troja said. "Magnetars are rapidly spinning neutron stars with huge magnetic fields. When they dump their magnetic power into the surroundings, they can make any explosion brighter and longer-lasting."
- [11]
Discovering more of these extreme X-ray flashes could help astronomers determine how often magnetars are formed through neutron star mergers, Passaleva said.
- [12]
Neutron star collisions forge elements like gold, silver and platinum.
- [13]
A collapsing stellar core can spin up a neutron star to over 700 times per second; magnetic fields get stronger when field lines are pushed closer together, so the collapse of a core with an already powerful field can create a neutron star with the strongest magnetic field in the universe, called a magnetar.
- [14]
The team's research was published in the journal Science Bulletin.
- [15]
"When I saw the X-ray data from this new event, I realized something was up," said Eleonora Troja, part of the Einstein Probe European collaboration.
- [16]
The 10-minute X-ray emission lasted about 1,200 times as long as the half-second gamma-ray burst.
Sources
1 independent publisher whose own reporting we read for this story.
- space.comMysterious 10-minute X-ray burst from a distant galaxy may have come from 2 dead stars colliding
1 article · October 9, 2026
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