X. Zhang

activity

20102024

most citedObservations of the luminous red nova AT 2021biy in the nearby galaxy NGC 4631

26 citations · 71 across the 5 of their papers we have counts for

collaborators

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3 papers · 1 filter

nucl-ex2024

Charge radii of $^{11 - 16}$ C, $^{13 - 17}$ N and $^{15 - 18}$ O determined from their charge-changing cross-sections and the mirror-difference charge radii

J. W. Zhao, B. -H. Sun, I. Tanihata +24

Charge-changing cross-sections of $^{11 - 16}$ C, $^{13 - 17}$ N and $^{15 - 18}$ O on a carbon target have been determined at energies around 300 MeV/nucleon. A nucleon separation energy-d…

nucl-ex2023★ 24 cited

Isospin-dependence of the charge-changing cross-section shaped by the charged-particle evaporation process

J. W. Zhao, B. -H. Sun, I. Tanihata +26

We present the charge-changing cross sections (CCCS) of $^{11 - 15}$ C, $^{13 - 17}$ N, and $^{15, 17 - 18}$ O at around 300 MeV/nucleon on a carbon target, which extends to $p$ -shell isotop…

nucl-ex2010

Investigation of excited states in $^{18}$ Ne via resonant elastic scattering of $^{17}$ F+p and its astrophysical implication in the stellar reaction of $^{14}$ O( $α$ , $p$ ) $^{17}$ F

J. Hu, J. J. He, S. W. Xu +35

Properties of proton resonances in $^{18}$ Ne have been investigated efficiently by utilizing a technique of proton resonant elastic scattering with a $^{17}$ F radioactive ion (RI)…

Charge radii of 11−16C, 13−17N and 15−18O determined from their charge-changing cross-sections and the mirror-difference charge radii

Isospin-dependence of the charge-changing cross-section shaped by the charged-particle evaporation process

Investigation of excited states in 18Ne via resonant elastic scattering of 17F+p and its astrophysical implication in the stellar reaction of 14O(α,p)17F

Charge radii of $^{11 - 16}$ C, $^{13 - 17}$ N and $^{15 - 18}$ O determined from their charge-changing cross-sections and the mirror-difference charge radii

Investigation of excited states in $^{18}$ Ne via resonant elastic scattering of $^{17}$ F+p and its astrophysical implication in the stellar reaction of $^{14}$ O( $α$ , $p$ ) $^{17}$ F