The birth of radio millisecond pulsars and their high-energy signature

P. H.T. Tam, K. L. Li, A. K.H. Kong, J. Takata, G. C.K. Leung, K. S. Cheng, C. Y. Hui

研究成果: Conference article同行評審

摘要

Millisecond pulsars (MSPs) are thought to born in low-mass X-ray binaries when the neutron star has gained enough angular momentum from the accreting materials of its companion star. It is generally believed that a radio MSP is born when the neutron star stops accreting and enters a rotation-powered state. Exactly what happens during the transition time was poorly understood until a year ago. In the past year, observations have revealed a few objects that not only switched from one state to the other (as predicted in the above picture), but also have swung between the two states within weeks to years. In this work, we present observations of two of these transition objects (PSR J1023+0038 and XSS J12270-4859) and a theoretical framework that tries to explain their high-energy radiation.

原文English
期刊Proceedings of Science
228
出版狀態Published - 2014
事件10th INTEGRAL Workshop: "A Synergistic View of the High Energy Sky", Integral 2014 - Annapolis, United States
持續時間: 2014 九月 152014 九月 19

All Science Journal Classification (ASJC) codes

  • 多學科

指紋

深入研究「The birth of radio millisecond pulsars and their high-energy signature」主題。共同形成了獨特的指紋。

引用此