176 citations · 853 across the 45 of their papers we have counts for
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Two types of glitches in a solid quark star model
Jiguang Lu, Enping Zhou
TThe glitch of anomalous X-ray pulsars \& soft gamma repeaters (AXP/SGRs) usually accompanied with detectable energy releases manifesting as X-ray bursts or outbursts, while the gl…
The Magnetic Field Evolution of ULX NuSTAR J095551+6940.8 in M82--A Legacy of Accreting Magnetar
Y. Y. Pan, L. M. Song, C. M. Zhang +1
Ultra-luminous X-ray sources are usually believed to be black holes with mass about . However, the recent discovery of NuSTAR J095551+6940.8 in M82 by Bachetti e…
Ultraluminous X-ray pulsar: accreting magnetar?
H. Tong
Magnetars are a special kind of neutron stars. There may also be accreting magnetars. From the studies of isolated magnetars, it is known that a neutron star with a strong dipole f…
Massive Pulsars and Ultraluminous X-ray Sources
Yanjun Guo, Hao Tong, Renxin Xu
The detection of 1.37s pulsations from NuSTAR J095551+6940.8 implies the existence of an accreting pulsar, which challenges the conventional understanding of ultraluminous X-r…
On the variable timing behavior of PSR B0540-69: an almost excellent example to study pulsar braking mechanism
F. F. Kou, Z. W. Ou, H. Tong
PSR B0540-69 has braking index measurement in its persistent state: n=2.129 \pm 0.012. Recently, it is reported to have spin-down state changes: a suddenly 36 % increase in the spi…
Two types of glitches in a solid quark star model
Enping Zhou
Glitch (sudden spinup) is a common phenomenon in pulsar observations. However, the physical mechanism of glitch is still a matter of debate because it depends on the puzzle of puls…