期刊论文

Yu, Yun-Wei（俞云伟）

英文

ASTROPHYSICAL JOURNAL

0004-637X

2021

907

2

87

10.3847/1538-4357/abcc70

National SKA Program of China [2020SKA0120300]; National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC) [11822302, 11833003, 11722324, 11690024, 11633001]; Strategic Priority Research Program of the Chinese Academy of SciencesChinese Academy of Sciences [XDB23040100]

本校为通讯机构

A rapidly rotating and highly magnetized neutron star (NS) could be formed from explosive phenomena such as superluminous supernovae and gamma-ray bursts. This newborn NS can substantially influence the emission of these explosive transients through its spin-down. The spin-down evolution of the NS can sometimes be affected by fallback accretion, although it is usually regulated by the magnetic dipole radiation and gravitational wave radiation of the NS. Under appropriate conditions, the accreting material can be first ejected and subsequently recycled back, so that the accretion disk can remai...