Magnetar-like X-Ray Bursts Suppress Pulsar Radio Emission

被引：24

作者：

Archibald, R. F. ^{[1
,2
,3
]}

Burgay, M. ^{[4
]}

Lyutikov, M. ^{[1
,2
,5
]}

Kaspi, V. M. ^{[1
,2
]}

Esposito, P. ^{[6
]}

Israel, G. ^{[7
]}

Kerr, M. ^{[8
]}

Possenti, A. ^{[4
]}

Rea, N. ^{[6
,9
]}

Sarkissian, J. ^{[10
]}

Scholz, P. ^{[11
]}

Tendulkar, S. P. ^{[1
,2
]}

机构：

[1] McGill Univ, Dept Phys, 3600 Univ St, Montreal, PQ H3A 2T8, Canada

[2] McGill Univ, McGill Space Inst, 3600 Univ St, Montreal, PQ H3A 2T8, Canada

[3] Univ Toronto, Dept Astron & Astrophys, 50 St George St, Toronto, ON M5S 3H4, Canada

[4] INAF Osservatorio Astron Cagliari, Via Sci 5, I-09047 Selargius, Italy

[5] Purdue Univ, Dept Phys, 525 Northwestern Ave, W Lafayette, IN 47907 USA

[6] Univ Amsterdam, Anton Pannekoek Inst Astron, Postbus 94249, NL-1090 GE Amsterdam, Netherlands

[7] INAF Osservatorio Astron Roma, Via Frascati 33, I-00040 Rome, Italy

[8] US Navy, Res Lab, Space Sci Div, Washington, DC 20375 USA

[9] Inst Space Sci ICE CSICIEEC, Carrer Can Magrans S-N, E-08193 Barcelona, Spain

[10] CSIRO Astron & Space Sci, Parkes Observ, POB 276, Parkes, NSW 2870, Australia

[11] Natl Res Council Canada, Herzberg Astron & Astrophys, Domin Radio Astrophys Observ, POB 248, Penticton, BC V2A 6J9, Canada

来源：

ASTROPHYSICAL JOURNAL LETTERS | 2017年 / 849卷 / 02期

基金：

加拿大自然科学与工程研究理事会; 美国国家航空航天局; 美国国家科学基金会;

关键词：

pulsars: general; pulsars: individual (PSR J1119-6127); stars: magnetars; SUPERNOVA REMNANT G292.2-0.5; PSR J1119-6127; FIELD; ORIGIN; HOST;

D O I：

10.3847/2041-8213/aa9371

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Rotation-powered pulsars and magnetars are two different observational manifestations of neutron stars: rotationpowered pulsars are rapidly spinning objects that are mostly observed as pulsating radio sources, while magnetars, neutron stars with the highest known magnetic fields, often emit short-duration X-ray bursts. Here, we report simultaneous observations of the high-magnetic-field radio pulsar PSR. J1119-6127 at X-ray, with XMM-Newton and NuSTAR, and at radio energies with the Parkes radio telescope, during a period of magnetar-like bursts. The rotationally powered radio emission shuts off coincident with the occurrence of multiple X-ray bursts and recovers on a timescale of similar to 70. s. These observations of related radio and X-ray phenomena further solidify the connection between radio pulsars and magnetars and suggest that the pair plasma produced in bursts can disrupt the acceleration mechanism of radio-emitting particles.

引用

页数：5

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