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PSR B1937+21 is a millisecond pulsar located in the direction of the constellation Vulpecula, renowned for its astonishing rotation speed of 642 revolutions per second. Since its discovery in 1982, it ...
A breakthrough in nuclear physics at Florida Polytechnic University has created an advanced machine learning model that ...
Morning Overview on MSN
Astronomers detect repeating fast radio bursts near milky way black hole
Recent discoveries by astronomers have revealed the presence of repeating fast radio bursts (FRBs) emanating from a region ...
They're oddballs of the transmission world, but they're great for moving a powerful drag racer at super-high speeds. Here's ...
Discovered in 1982, PSR B1937+21 is one of the first millisecond pulsars, with an ultra-short period of 1.558 milliseconds ...
The Oak Ridger on MSN
Next ORION meeting is Sept. 17 at Roane State's Oak Ridge campus
The title of the program is “The Lightest and Heaviest Elements and their Isotopes as Powerful Groundater Tracers.” The ...
Knowable Magazine reports that neutrinos may help explain the universe's missing antimatter, shedding light on ...
On January 14, 2025, a gravitational wave dubbed GW250114 reached Earth. Like its predecessor, GW150914, it came from a pair ...
22hon MSN
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 ...
Celestium on MSN
What Makes Neutron Stars the Most Extreme Objects in Space
Delve into the enigmatic realm of neutron stars—stellar remnants that defy our conventional understanding. Once blazing stars ...
Binary star systems are not rare. Neither are systems where one star is a remnant like a white dwarf or neutron star, and its companion is on the main sequence. In those systems, the dense remnant can ...
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