报告摘要：Among the binary millisecond pulsar populations, there is a group of millisecond pulsars with ultralight companions (referred to as spider pulsars) or extremely low mass (ELM) He white dwarfs (WDs). These systems with WD companions, are the progenitors of ultra-compact X-ray binaries that serve as important gravitational wave sources. However, the formation and evolution of these systems are not well understood. In this talk, I will talk about the binary formation model of spider pulsars and the discovery of the spider pulsar M71E with FAST. Subsequently, I will talk about the formation and evolution of binary millisecond pulsars with ELM WDs, along with a discussion of the properties of these systems as gravitational wave sources.

个人简介：陈海亮，研究员, 硕士生导师，主要从事致密双星的形成和演化、星族合成研究。2006-2010年云南大学本科；2010-2016云南天文台研究生，期间2013.1-2016.12马普天体物理研究所联合培养；2017-2022年中国科学院云南天文台副研究员，期间2019-2020年丹麦奥胡斯大学博士后（因疫情中断）；2022.9-中国科学院云南天文台研究员，已经发表论文SCI论文三十多篇，主持和参与多项国家基金。