activity
20212026
most citedA Morphological Classification of 18190 Molecular Clouds Identified in CO Data from the MWISP Survey

27 citations · 51 across the 18 of their papers we have counts for

collaborators
Showing 2024Show all

6 papers · 1 filter

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.…