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X-ray Flares from Postmerger Millisecond Pulsars

Open access
Dai, Z. G., Wang, X. Y., Wu, X. F., Zhang, B.·2006·Science

Abstract

Recent observations support the suggestion that short-duration gamma-ray bursts are produced by compact star mergers. The x-ray flares discovered in two short gamma-ray bursts last much longer than the previously proposed postmerger energy-release time scales. Here, we show that they can be produced by differentially rotating, millisecond pulsars after the mergers of binary neutron stars. The differential rotation leads to windup of interior poloidal magnetic fields and the resulting toroidal fields are strong enough to float up and break through the stellar surface. Magnetic reconnection–driven explosive events then occur, leading to multiple x-ray flares minutes after the original gamma-ray burst.

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Metadata

Authors
Dai, Z. G., Wang, X. Y., Wu, X. F., & Zhang, B.
Venue
Science
Published
2006-02-24
Volume
311
Issue
5764
Pages
1127-1129
ISSN
  • 0036-8075 (ISSN-L)
  • 1095-9203
OpenAlex
W2072292705
Cited by
365
References
0
FWCI
11.38
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: X-ray Flares from Postmerger Millisecond Pulsars. https://app.cochat.ai/papers/10.1126/science.1123606
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Dai, Z. G., Wang, X. Y., Wu, X. F., & Zhang, B. (2006). X-ray Flares from Postmerger Millisecond Pulsars. Science. https://doi.org/10.1126/science.1123606

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.