activity
20242026
collaborators

9 papers

astro-ph.GA2026

Correlation between the two-armed spiral in the -- plane and moving groups

Yan Xu, Chao Liu, Chengdong Li +5

We use a cross-matched sample of 3.7 million stars from Gaia DR3 and LAMOST DR7 to investigate the velocity substructures in the Milky Way disk. The median radial velocity as…

astro-ph.SR2026

A Search for High Frequency Oscillations in TESS Cycle 7

Guanda Huang, Xiaodian Chen, Shu Wang +2

High-quality, short-cadence photometry from TESS enables the detection of rapid oscillators with unprecedented sensitivity. In this work, we conduct a homogeneous search for high-f…

astro-ph.GA2026

The extinction distances for over a thousand planetary nebulae with Gaia measurements

Juan Deng, Shu Wang, Biwei Jiang +1

Although Gaia has identified the central stars of planetary nebulae (CSPNe) for about 70% of known Galactic planetary nebulae (PNe), reliable distance estimates remain incomplete,…

astro-ph.SR2025

Classification for 969 double-mode RR Lyrae stars from Zwicky Transient Facility

Jianxing Zhang, Xiaodian Chen, Shu Wang +2

RR Lyrae (RRL) variable stars are cornerstone distance indicators. In particular, double-mode RR Lyrae (RRd) stars enable period--luminosity relations (PLRs) that are less sensitiv…

astro-ph.GA2025

A Detailed Analysis of the Milky Way Warp Based on Classical Cepheids

Xiaoyue Zhou, Xiaodian Chen, Licai Deng +3

Classical Cepheids (CCs) are important probes for the large-scale warp structure of the Milky Way. Using Gaia DR3 CCs, we establish an optimal time-dependent warp model, where the…

astro-ph.SR2025

A search of periodic variable stars in the LMC by JWST photometry

Jiyu Wang, Xiaodian Chen, Jianxing Zhang +3

Based on high-resolution near-infrared photometric data from the James Webb Space Telescope (JWST) targeting the Large Magellanic Cloud (LMC), this study attempts to evaluate the f…