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A repeating fast radio burst
Dan Delany
post Mar 3 2016, 01:42 AM
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A repeating fast radio burst

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Fast radio bursts are millisecond-duration astronomical radio pulses of unknown physical origin that appear to come from extragalactic distances. Previous follow-up observations have failed to find additional bursts at the same dispersion measure (that is, the integrated column density of free electrons between source and telescope) and sky position as the original detections. The apparent non-repeating nature of these bursts has led to the suggestion that they originate in cataclysmic events. Here we report observations of ten additional bursts from the direction of the fast radio burst FRB 121102. These bursts have dispersion measures and sky positions consistent with the original burst. This unambiguously identifies FRB 121102 as repeating and demonstrates that its source survives the energetic events that cause the bursts. Additionally, the bursts from FRB 121102 show a wide range of spectral shapes that appear to be predominantly intrinsic to the source and which vary on timescales of minutes or less. Although there may be multiple physical origins for the population of fast radio bursts, these repeat bursts with high dispersion measure and variable spectra specifically seen from the direction of FRB 121102 support an origin in a young, highly magnetized, extragalactic neutron star.


More exciting FRB news! I wonder if this is likely to be a member of a different class of FRBs, with a different origin story, than the one-off events detected previously? Or if many of the others have also had additional bursts that have just gone undetected? Perhaps a little of both.
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Mongo
post Mar 3 2016, 09:28 PM
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That's fascinating, and quite puzzling to me. Considering the enormous amounts of energy that each FRB must consume to be detectable at extragalactic distances, I'm surprised to see what appears to be an object that emits repeated FRBs. I suspect that this object is a lot closer than the first localized FRB at 6 billion LY. That one was apparently a pair of colliding neutron stars. I guess that this one is maybe in near-extragalactic space, within a few million LY of us, and the mechanism is a lot less energetic than two colliding neutron stars.
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TheAnt
post Mar 6 2016, 12:53 AM
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QUOTE (Mongo @ Mar 3 2016, 10:28 PM) *
......and the mechanism is a lot less energetic than two colliding neutron stars.


Perhaps they don't collide properly, but merely bounce against each other! wacko.gif
(Sorry couldn't resist.)
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