activity
20202026
most citedLocal Spiral Structure Traced by Red Clump Stars

22 citations · 70 across the 23 of their papers we have counts for

collaborators

23 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.HE2025★ 1 cited

Detection and Characterization of Quasi-Periodic Oscillations in Seyfert Galaxy NGC 4151

Yan Yongkang, Zhang Peng, Lu Zhou +6

This study aims to detect and characterize quasi-periodic oscillations (QPOs) signals in X-ray observations of NGC 4151. We employed the Weighted Wavelet Z-transform (WWZ) and Lomb…

astro-ph.GA2025

Outflowing Gas in the Planetary Nebula K 3-54

Xiuhui Chen, Dejian Liu, Ping Yan +3

As planetary nebulae (PNe) evolve, they develop slow and strong dust-driven stellar winds, making the joint study of dust and gas essential for understanding their nature. As a pil…

astro-ph.GA2024

Kinematics of Young Stellar Objects Under Various Stellar Feedback

Longhui Yang, Dejian Liu, Chaojie Hao +6

Based on the Gaia Data Release 3 and APOGEE datasets, we investigate the kinematic differences between young stellar objects (YSOs) and their parent clouds in five nearby star-form…

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

Maser Investigation toward Off-Plane Stars (MIOPS): detection of SiO masers in the Galactic thick disk and halo

Wenjin Yang, Yuanwei Wu, Yan Gong +7

Studying stars that are located off the Galactic plane is important for understanding the formation history of the Milky Way. We searched for SiO masers toward off-plane O-rich asy…

astro-ph.GA2023

Kinematics of the Local Spiral Structure Revealed by Young Stars in \emph{Gaia}~DR3

Dejian Liu, Ye Xu, Chaojie Hao +4

Using young open clusters and O--B2-type stars in~\emph{Gaia}~DR3, we investigate the kinematics of the local spiral structure. In general, the young sources in the outer spiral ar…

astro-ph.GA2023★ 9 cited

Distributions and Physical Properties of Molecular Clouds in the Third Galactic Quadrant: = [219.75, 229.75] and = [-5.25, 5.25]

Yiwei Dong, Yan Sun, Ye Xu +11

We present the results of an unbiased CO/CO/CO ( = 1-0) survey in a portion of the third Galactic quadrant (TGQ): = [219.75, 229.75] and = […

astro-ph.SR2022★ 6 cited

Calibrating the Cepheid Period--Wesenheit Relation in the Gaia Bands using Galactic Open Cluster Cepheids

Zehao Lin, Ye Xu, Chaojie Hao +3

Establishing the period--Wesenheit relation requires independent and accurate distance measurements of classical Cepheids (DCEPs). The precise distance provided by an associated op…

gr-qc2022★ 8 cited

The Effect of Light Deflection by Solar System Objects on High-Precision SKA Astrometry

Yingjie Li, Ye Xu, Shaibo Bian +4

We have computed the deflection angles caused by 195 objects in the solar system, including 177 satellites and eight asteroids. Twenty-one satellites and six asteroids can bend lig…

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…

astro-ph.IM2022★ 5 cited

A baseline correction algorithm for FAST

De-Jian Liu, Ye Xu, Ying-Jie Li +3

The Five-hundred-meter Aperture Spherical radio Telescope (FAST) is the most sensitive ground-based, single-dish radio telescope on Earth. However, the original HI spectra produced…

astro-ph.GA2022★ 22 cited

Local Spiral Structure Traced by Red Clump Stars

Zehao Lin, Ye Xu, Ligang Hou +5

Using the cross-matched data of Gaia EDR3 and the 2MASS Point Source Catalog, a sample of RC stars with parallax accuracies better than 20% is identified and used to reveal the nea…

gr-qc2021

Light Deflection under the Gravitational Field of Jupiter -- Testing General Relativity

Yingjie Li, Ye Xu, JingJing Li +6

We measured the relative positions between two pairs of compact extragalactic sources (CESs), J1925-2219 \& J1923-2104 (C1--C2) and J1925-2219 \& J1928-2035 (C1--C3) on 2020 Octobe…

astro-ph.GA2020★ 8 cited

High-sensitivity millimeter imaging of molecular outflows in nine nearby high-mass star-forming regions

De-Jian Liu, Ye Xu, Ying-Jie Li +6

We present a study of molecular outflows using six molecular lines (including 12CO/13CO/C18O/HCO+(J = 1-0) and SiO/CS(J = 2-1)) toward nine nearby high-mass star-forming regions wi…