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XRISM found dense winds from a neutron star disc differ from those around black holes, challenging ideas on how such winds form and shape their environment.
On February 25, 2024, XRISM used its Resolve instrument to observe the neutron star GX13+1, which is the core of a once larger star that has burned out. GX13+1 is a bright X-ray source. These X-rays ...
On February 25, 2024, XRISM used its Resolve instrument to observe the neutron star GX13+1, which is the core of a once larger star that has burned out. GX13+1 is a bright X-ray source. These X-rays ...
New images have revealed the supermassive black hole at the center of galaxy M87 flipping its gravitational field.
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XRISM reveals surprisingly sluggish winds from neutron star differ from black hole outflows
The X-Ray Imaging and Spectroscopy Mission (XRISM) has revealed an unexpected difference between the powerful winds launching ...
Astronomers using the new X-Ray Imaging and Spectroscopy Mission (XRISM) have discovered that the fierce winds blowing from matter spiraling into a neutron star behave very differently from those ...
The X-Ray Imaging and Spectroscopy Mission (XRISM) has revealed an unexpected difference between the powerful winds launching from a disc around a ...
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Space scientists puzzled after black hole observed behaving in unexpected way
Space scientists are puzzled after discovering a black hole behaving in an unexpected way. New images have revealed the supermassive black hole at the centre of galaxy M87 flipping its gravitational ...
Astronomers using the Webb Telescope may have found a new type of object: cold, glowing black hole stars from the early ...
Most supermassive black holes lurk in the nuclei of galaxies, surrounded by stars and glowing with haloes of superhot matter, ...
Astronomers confirmed an off-center black hole in a dwarf galaxy. It offers clues to how supermassive black holes may form.
Astronomers at Penn State have nicknamed the objects “universe breakers,” which may be unusual black hole atmospheres and could represent a missing link in the fast growth of supermassive black holes.
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