7 citations · 7 across the 3 of their papers we have counts for
3 papers
astro-ph.HE2025
A statistical study of type II outbursts of XRPs: Brighter accreting pulsars rotate faster
Shan-Shan Weng, Xiao-Tian Xu, Han-Long Peng +6
X-ray pulsars (XRPs) consist of a magnetized neutron star (NS) and an optical donor star. The NS accretes matter from the donor star producing pulsed X-ray emission. In most cases…
astro-ph.HE2024
On the ultra-long spin period of 4U 1954+31
Ying-Han Mao, Xiang-Dong Li
4U 1954+31 is a high-mass X-ray binary (HMXB) that contains a neutron star and an M supergiant companion. The neutron star has a spin period of ~5.4 hr. The traditional wind-accret…
astro-ph.HE2023★ 7 cited
Back to the Starting Point: on the Simulation of Initial Magnetic Fields and Spin Periods of Non-accretion Pulsars
Kun Xu, Hao-Ran Yang, Ying-Han Mao +3
Neutron stars (NSs) play essential roles in modern astrophysics. Magnetic fields and spin periods of newborn (zero age) NSs have large impact on the further evolution of NSs, which…