Some pulsars spin very fast compared to others, with periods on the order of milliseconds. This article describes a study that identifies high-energy emissions in gamma-rays from millisecond pulsars. The results of this study can advance this line of research.
Address: 20A Datun Road, Chaoyang District, Beijing, China code: 100012
Tel: 010-64888708 E-mail: email@example.com