By studying the signal of GW170817 from the merger of two neutron stars and the result, including in a kilonova, a team of astronomers is identifying the unique nature of this phenomenon, including a residual X-ray stream that is likely to provide clues to the nature of this phenomenon.. The object resulting from The merger of these two massive stars.
Discovered on August 17, 2017 in It is a reference attributed to the direct realization of†Described as oscillations in curvature Albert predicted the propagation of gravitational waves from a source As early as 1916, it took nearly a hundred years for the first observation of gravitational waves to be made, in September 2015.NGC 4993 via Tools and the (two interferometers are designed to detect) †
according to † But what makes it special is its discovery Related: This is the first time an astronomical phenomenon in the form of gravitational waves and light has been detected. In fact, a Gamma (GRB170817A), associated with GW170817, is detected by: Less than two seconds after the start of the gravitational wave signal.Could this signal be issued yet? between two
Since then, nearly 70 observatories, on Earth or in space, have taken part in observing this phenomenon. The And VLBA can detect waves, for example Residues associated with GW170817, confirming the A. two †American
Kilonova is associated with this phenomenon
The AT 2017gfo event was detected about 11 hours after gravitational waves were observed (It can be defined as a file under the light). Due to its spatial and temporal proximity to GW170817, this kilonova was associated with the same neutron star merger. This phenomenon was accompanied by jets of rapidly moving charged particles. he moved close and production X-rays, measured by NASA’s Chandra Observatory. According to a team of American astrophysicists, the study of these X-rays could hold the key to identifying the object resulting from the merger of these two neutron stars.
Shortly after the discovery, X-rays are emitted from an aircraftIt will decrease little by little, while the flow of matter will slow down. But since 2020, this decline has occurred They stop and give way to a relatively steady X-ray. according to This then indicates the discovery of an additional object, other than the charged particle beam: a different X-ray source is therefore needed to explain these observations.
Aurora… or even a black hole?
, this new source of X-rays could come from a shock from the rapid expansion of debris from the merger between the two stars. This shock would have heated the surrounding material and thus would emit X-rays – a phenomenon that would then be associated with the Kilonova’s residual glow.
To find the end of the story, the They will continue to observe GW170817, both in X-rays and radio waves: in the case of the remaining brightness of a kilonova, X-rays and radio waves are expected to increase in the coming months. On the other hand, if the emission of X-rays decreased and the emission of radio waves stopped, scientists would lean toward the formation scenario instead. (This would then be the lowest mass detected!).
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