The X-ray counterpart to the gravitational-wave event GW170817

• Published in: Nature (London) Vol. 551; no. 7678; pp. 71 - 74
• Main Authors: Troja, E., Piro, L., van Eerten, H., Wollaeger, R. T., Im, M., Fox, O. D., Butler, N. R., Cenko, S. B., Sakamoto, T., Fryer, C. L., Ricci, R., Lien, A., Ryan, R. E., Korobkin, O., Lee, S.-K., Burgess, J. M., Lee, W. H., Watson, A. M., Choi, C., Covino, S., D’Avanzo, P., Fontes, C. J., González, J. Becerra, Khandrika, H. G., Kim, J., Kim, S.-L., Lee, C.-U., Lee, H. M., Kutyrev, A., Lim, G., Sánchez-Ramírez, R., Veilleux, S., Wieringa, M. H., Yoon, Y.
• Format: Journal Article
• Language: English
• Published: London Nature Publishing Group UK 02.11.2017; Nature Publishing Group
• Subjects: 639/33/34/864; 639/33/34/867; ASTRONOMY AND ASTROPHYSICS; Astrophysics; Bursting; Bursts; Collimation; counterpart; Ejecta; Ejection; Emission; Emissions; Gamma rays; Gravitational waves; Gravity; Humanities and Social Sciences; kilonova; letter; Light; multidisciplinary; Neutron stars; Neutrons; Nuclear capture; Observations; Observatories; r-process; Radio frequency; Relativism; Science; Star & galaxy formation; X-ray emissions; X-rays
• ISSN: 0028-0836; 1476-4687
• DOI: 10.1038/nature24290

Detection of X-ray emission at a location coincident with the kilonova transient of the gravitational-wave event GW170817 provides the missing observational link between short gamma-ray bursts and gravitational waves from neutron-star mergers. When neutron stars collide Merging neutron stars are potential sources of gravitational waves and have long been predicted to produce jets of material as part of a low-luminosity transient known as a 'kilonova'. There is growing evidence that neutron-star mergers also give rise to short, hard gamma-ray bursts. A group of papers in this issue report observations of a transient associated with the gravitational-wave event GW170817—a signature of two neutron stars merging and a gamma-ray flash—that was detected in August 2017. The observed gamma-ray, X-ray, optical and infrared radiation signatures support the predictions of an outflow of matter from double neutron-star mergers and present a clear origin for gamma-ray bursts. Previous predictions differ over whether the jet material would combine to form light or heavy elements. These papers now show that the early part of the outflow was associated with lighter elements whereas the later observations can be explained by heavier elements, the origins of which have been uncertain. However, one paper (by Stephen Smartt and colleagues) argues that only light elements are needed for the entire event. Additionally, Eleonora Troja and colleagues report X-ray observations and radio emissions that suggest that the 'kilonova' jet was observed off-axis, which could explain why gamma-ray-burst detections are seen as dim. A long-standing paradigm in astrophysics is that collisions—or mergers—of two neutron stars form highly relativistic and collimated outflows (jets) that power γ-ray bursts of short (less than two seconds) duration 1 , 2 , 3 . The observational support for this model, however, is only indirect 4 , 5 . A hitherto outstanding prediction is that gravitational-wave events from such mergers should be associated with γ-ray bursts, and that a majority of these bursts should be seen off-axis, that is, they should point away from Earth 6 , 7 . Here we report the discovery observations of the X-ray counterpart associated with the gravitational-wave event GW170817. Although the electromagnetic counterpart at optical and infrared frequencies is dominated by the radioactive glow (known as a ‘kilonova’) from freshly synthesized rapid neutron capture (r-process) material in the merger ejecta 8 , 9 , 10 , observations at X-ray and, later, radio frequencies are consistent with a short γ-ray burst viewed off-axis 7 , 11 . Our detection of X-ray emission at a location coincident with the kilonova transient provides the missing observational link between short γ-ray bursts and gravitational waves from neutron-star mergers, and gives independent confirmation of the collimated nature of the γ-ray-burst emission.