activity
20182022
most citedMost Lithium-rich Low-mass Evolved Stars Revealed as Red Clump stars by Asteroseismology and Spectroscopy

59 citations · 224 across the 7 of their papers we have counts for

collaborators

8 papers

astro-ph.SR202250 cited

Discovery of post-mass-transfer helium-burning red giants using asteroseismology

Yaguang Li, Timothy R. Bedding, Simon J. Murphy +14

A star expands to become a red giant when it has fused all the hydrogen in its core into helium. If the star is in a binary system, its envelope can overflow onto its companion or…

astro-ph.SR202118 cited

Lithium Evolution of Giant Stars Observed by LAMOST and Kepler

Jinghua Zhang, Jian-Rong Shi, Hong-Liang Yan +8

Mapping lithium evolution for evolved stars will provide restrictions and constraints on the fundamental stellar interior physical processes, which further shed light on our unders…

astro-ph.SR20204 cited

Mode Angular Degree Identification in Subgiant Stars with Convolutional Neural Networks based on Power Spectrum

Minghao Du, Shaolan Bi, Xianfei Zhang +3

Identifying the angular degrees of oscillation modes is essential for asteroseismology and depends on visual tagging before fitting power spectra in a so-called peakbagging ana…

astro-ph.SR202059 cited

Most Lithium-rich Low-mass Evolved Stars Revealed as Red Clump stars by Asteroseismology and Spectroscopy

Hong-Liang Yan, Yu-Tao Zhou, Xianfei Zhang +19

Lithium has confused scientists for decades at almost each scale of the universe. Lithium-rich giants are peculiar stars with lithium abundances over model prediction. A large frac…

astro-ph.HE202024 cited

What binary systems are the most likely sources for periodically repeating FRBs?

Xianfei Zhang, He Gao

The newly discovered 16.35 days period for repeating FRB 180916.J0158+65 provides an essential clue for understanding the sources and emission mechanism of repeating FRBs. Many mod…

astro-ph.SR202020 cited

Solar-type Stars Observed by LAMOST and Kepler

Jinghua Zhang, Alexander I. Shapiro, Shaolan Bi +8

Obtaining measurements of chromospheric and photometric activity of stars with near-solar fundamental parameters and rotation periods is important for a better understanding of sol…