A magnetar-powered X-ray transient as the aftermath of a binary neutron-star merger

Y. Q. Xue, X. C. Zheng, Y. Li, W. N. Brandt, B. Zhang, B. Luo, B. B. Zhang, F. E. Bauer, H. Sun, B. D. Lehmer, X. F. Wu, G. Yang, X. Kong, J. Y. Li, M. Y. Sun, J. X. Wang, F. Vito

Research output: Contribution to journalArticlepeer-review

34 Scopus citations

Abstract

Mergers of neutron stars are known to be associated with short γ-ray bursts1–4. If the neutron-star equation of state is sufficiently stiff (that is, the pressure increases sharply as the density increases), at least some such mergers will leave behind a supramassive or even a stable neutron star that spins rapidly with a strong magnetic field5–8 (that is, a magnetar). Such a magnetar signature may have been observed in the form of the X-ray plateau that follows up to half of observed short γ-ray bursts9,10. However, it has been expected that some X-ray transients powered by binary neutron-star mergers may not be associated with a short γ-ray burst11,12. A fast X-ray transient (CDF-S XT1) was recently found to be associated with a faint host galaxy, the redshift of which is unknown13. Its X-ray and host-galaxy properties allow several possible explanations including a short γ-ray burst seen off-axis, a low-luminosity γ-ray burst at high redshift, or a tidal disruption event involving an intermediate-mass black hole and a white dwarf13. Here we report a second X-ray transient, CDF-S XT2, that is associated with a galaxy at redshift z = 0.738 (ref. 14). The measured light curve is fully consistent with the X-ray transient being powered by a millisecond magnetar. More intriguingly, CDF-S XT2 lies in the outskirts of its star-forming host galaxy with a moderate offset from the galaxy centre, as short γ-ray bursts often do15,16. The estimated event-rate density of similar X-ray transients, when corrected to the local value, is consistent with the event-rate density of binary neutron-star mergers that is robustly inferred from the detection of the gravitational-wave event GW170817.

Original languageEnglish (US)
Pages (from-to)198-201
Number of pages4
JournalNature
Volume568
Issue number7751
DOIs
StatePublished - Apr 11 2019

All Science Journal Classification (ASJC) codes

  • General

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