作者: Giancarlo Cusumano , Maria C Maccarone , Luciano Nicastro , Bruno Sacco , Phil Kaaret
DOI: 10.1063/1.1303201
关键词: Spin-½ 、 Astronomy 、 Stellar rotation 、 X-ray binary 、 X-ray 、 Pulsar 、 Binary system 、 Physics 、 Astrophysics 、 Neutron star 、 Binary number
摘要: We have detected 33.8 ms pulsations from SAX J0635+0533, a newly discovered Be/X-ray binary suggested as possible counterpart to the gamma-ray source 2EG J0635+0521. interpret periodicity spin period of neutron star in system with Be companion.