7 citations · 8 across the 2 of their papers we have counts for
4 papers
NuSTAR and XMM-Newton observations of SXP 59 during its 2017 giant outburst
Shan-Shan Weng, Ming-Yu Ge, Hai-Hui Zhao
The Be X-ray pulsar (BeXRP) SXP 59 underwent a giant outburst in 2017 with a peak X-ray luminosity of erg~s. We report on the X-ray behaviour of SXP 59 wi…
The scaling relation and its difference between cool-core and non-cool-core clusters
Yue Zhu, Yuan-Hao Wang, Hai-Hui Zhao +3
We construct a sample of 70 clusters using data from XMM-Newton and Planck to investigate the scaling relation and the cool-core influences on t…
Recurrent outbursts revealed in 3XMM J031820.8-663034
Hai-Hui Zhao, Shan-Shan Weng, Jun-Xian Wang
3XMM J031820.8-663034, first detected by ROSAT in NGC 1313, is one of a few known transient ultraluminous X-ray sources (ULXs). In this paper, we present decades of X-ray data of t…
Pulse phase-resolved analysis of SMC X-3 during its 2016--2017 super-Eddington outburst
Hai-Hui Zhao, Shan-Shan Weng, Ming-Yu Ge +2
The Be X-ray pulsar SMC X-3 underwent an extra long and ultraluminous giant outburst from 2016 August to 2017 March. The peak X-ray luminosity is up to erg/s, sugges…