activity
20222026
most citedSearch for Classical Cepheids in Galactic Open Clusters and Calibration of the Period Wesenheit Metallicity Relation in the Gaia Bands

8 citations · 15 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.GA2026

High-Priority Compact-Object Candidates in Young Clusters from the \textit{Gaia} DR3 Non-Single-Star Catalog

Dejian Liu, Kangteng Chang, Yao Huang +7

The search for massive compact objects such as black holes (BHs) or neutron stars (NSs) in star clusters is longstanding challenge in astrophysics, yet no definitive identification…

astro-ph.GA2026

Star Formation in the H II Region Sh 2-205: 3D Morphology and Kinematics from Young Stars and Molecular Gas

Yiwei Dong, Chaojie Hao, Ye Xu +5

Using Gaia astrometry of young stars combined with CO observations, we present the first systematic three-dimensional (3D) analysis of the structure, kinematics, and evolutionary h…

astro-ph.GA2026

Mapping the Milky Way with Masers

Ye Xu, Kazi Rygl, Huib Jan van Langevelde +10

SKA-VLBI is poised to revolutionize our understanding of the Galactic structure through its unprecedented astrometric precision and sensitivity. As a next-generation facility, it w…

astro-ph.GA2026

East Asian VLBI Network astrometry toward the star-forming region G040.96+02.48 in the Extreme Outer Galaxy

Xianjin Shen, Zehao Lin, Nobuyuki Sakai +18

Accurate astrometric measurements for star-forming regions located on the far side of the Milky Way remain scarce. In this work, we present the astrometric results for a 22\,GHz wa…

astro-ph.GA2025

Discovery of a high-velocity cloud of the Milky Way as a potential dark galaxy

Xiao-Lan Liu, Jin-Long Xu, Peng Jiang +6

High-velocity clouds (HVCs) are composed of neutral hydrogen (HI) moving at velocities that deviate from the general rotational motion of the Milky Way. Currently, the origins of t…

astro-ph.GA2024

A New Statistical Analysis of the Morphology of Spiral Galaxies

Junye Wei, Ye Xu, Zehao Lin +4

Morphology is the starting point for understanding galaxies. Elmegreen et al. classified spiral galaxies into flocculent, multiple-arm, and grand-design galaxies based on the regul…

astro-ph.GA2024

3D Morphology and Motions of the Canis Major Region from Gaia DR3

Yiwei Dong, Ye Xu, Chaojie Hao +4

The Canis Major (CMa) region is known for its prominent arc-shaped morphology, visible at multiple wavelengths. This study integrates molecular gas data with high-precision astrome…

astro-ph.SR2024★ 8 cited

Search for Classical Cepheids in Galactic Open Clusters and Calibration of the Period Wesenheit Metallicity Relation in the Gaia Bands

Huajian Wang, Ye Xu, Zehao Lin +3

It is beneficial to calibrate the period Wesenheit metallicity relation (PWZR) of Delta Cephei stars (DCEPs), i.e., classical Cepheids, using accurate parallaxes of associated open…

astro-ph.GA2024

VLBI with SKA: Possible Arrays and Astrometric Science

Yingjie Li, Ye Xu, Jingjing Li +4

The next generation of very long baseline interferometry (VLBI) is stepping into the era of microarcsecond (as) astronomy, and pushing astronomy, especially astrometry, to new h…

astro-ph.GA2024

Molecular Bubble and Outflow in S Mon Revealed by Multiband Datasets

Dejian Liu, Ye Xu, YingJie Li +8

We identify a molecular bubble, and study the star formation and its feedback in the S Mon region, using multiple molecular lines, young stellar objects (YSOs), and infrared data.…

astro-ph.GA2023★ 4 cited

Unveiling the initial conditions of open star cluster formation

C. J. Hao, Y. Xu, L. G. Hou +2

Open clusters (OCs) are infrequent survivors of embedded clusters gestated in molecular clouds. Up to now, little is known about the initial conditions for the formation of OCs. He…

astro-ph.GA2022

Neutral Stellar Winds Toward the High-Mass Star-Forming Region G176.51+00.20

Li Yingjie, Xu Ye, Xu Jin-Long +7

We observed the high-mass star-forming region G176.51+00.20 using the Five-hundred-meter Aperture Spherical radio Telescope (FAST) with the 19-beam tracking observational mode. Thi…

astro-ph.GA2022★ 3 cited

HI Narrow-Line Self-Absorptions Toward the High-Mass Star-Forming Region G176.51+00.20

Li Yingjie, Xu Ye, Xu Jin-Long +7

Using the Five-hundred-meter Aperture Spherical radio Telescope (FAST) 19-beam tracking observational mode, high sensitivity and high-velocity resolution HI spectral lines have bee…