演講資訊

摘要：

Accreting Millisecond X-Ray Pulsars (AMXPs) are astrophysical laboratories without parallel in the study of extreme physics. In this Colloquium/talk I report the past fifteen years of discoveries in this field. I will summarize the pulsar evolutionary prediction; how young and slow rotating pulsars end as old recycled fast millisecond pulsars “recycling model”. This long predicted model has been finally confirmed observationally step by step in the 15 past years. In addition, I review all kind of astrophysics aspect observed in accretion these accreting millisecond X-ray pulsars.