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Showing posts with the label neutron star collision

Hello, Multi-Messenger Astronomy!

As we posted Monday , it has certainly been a busy season for the scientists behind the Laser Interferometer Gravitational-Wave Observatory ( LIGO ) and its European counterpart, Virgo. Yesterday’s announcement of a neutron star merger is especially exciting because it’s the first detection made with gravitational waves that could also be viewed using optical telescopes. Within just a few hours of the initial gravitational wave detection and the gamma ray burst that arrived 1.5 seconds later, telescopes all over the world began to focus their gaze on the same region of the sky, catching a multispectral “ kilonova ” in action. “It was this extraordinary 2-to-3 day period,” said Aidan Brooks, staff scientist at the California Institute of Technology working on LIGO. “Everybody was completely elated and we just had this sort of amazing science flow in immediately after making this detection.”

A Neutron Star Collision: Gamma Rays & Gravitational Waves

Gravitational waves have been on our radar non-stop lately, from LIGO's fourth reported detection —enhanced by data from Italy's Virgo project —to this year's physics Nobel going to three of LIGO's cofounders. But here we are again and, far from getting old, the news is more exciting than ever: we've picked up a new kind of signal, from merging neutron stars rather than black holes. That's not all, though—while black hole mergers are expected to be difficult or impossible to see, this collision produced electromagnetic waves across a broad portion of the spectrum, allowing multiple telescopes to pick up the signal and giving us our first confirmed glimpse of a binary neutron star system coalescing into a single object.