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Yi-Yan Yang

Researcher at Chinese Academy of Sciences

Publications -  23
Citations -  162

Yi-Yan Yang is an academic researcher from Chinese Academy of Sciences. The author has contributed to research in topics: Neutron star & Pulsar. The author has an hindex of 7, co-authored 18 publications receiving 96 citations. Previous affiliations of Yi-Yan Yang include Beijing Normal University.

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Journal ArticleDOI

Hot disk of the Swift J0243.6+6124 revealed by Insight-HXMT

V. Doroshenko, +119 more
TL;DR: In this paper, a sharp state transition of the timing and spectral properties of the source at super-Eddington accretion rates was observed for magnetized X-ray pulsars.
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Fast radio bursts: do repeaters and non-repeaters originate in statistically similar ensembles?

TL;DR: In this article, the authors investigated the statistical classifications for the two groups of samples to see if the non-repeating and repeating FRBs have different origins by employing Anderson-Darling (A-D) test and Mann-Whitney-Wilcoxon (M-W-W) test.
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Similarity of PSR J1906+0746 to PSR J0737–3039: a Candidate of a New Double Pulsar System?

TL;DR: In this article, the authors compared the orbital parameters of PSR J1906+0746 with those of double pulsar systems and concluded that both systems have a similar origin and evolution history, involving an e-capture process for forming the second-born neutron star.
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Joint analysis of energy and RMS spectra from MAXI J1535-571 with Insight-HXMT

TL;DR: In this article, the authors performed a joint spectral analysis (2-150 keV) in both energy and time domains using observations taken by the first Chinese X-ray satellite, the Insight-HXMT, and showed that during the intermediate state, the energy spectra are in general consistent with those reported by Swift/XRT and NuSTAR.
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The mass distribution of Galactic double neutron stars: constraints on the gravitational-wave sources like GW170817

TL;DR: In this article, the authors applied a Bayesian analysis and Markov chain Monte Carlo simulation to 15 Galactic DNS systems, and obtained that the component masses of DNS systems should mainly fall in the range of 1.165-1.590