Yiwei Dong

most citedDistributions and Physical Properties of Molecular Clouds in the Third Galactic Quadrant:

l

= [219.75, 229.75]

^{\circ}

and

b

= [-5.25, 5.25]

^{\circ}

9 citations · 9 across the 3 of their papers we have counts for

collaborators

3 papers

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

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★ 9 cited

Distributions and Physical Properties of Molecular Clouds in the Third Galactic Quadrant: $l$ = [219.75, 229.75] $^{\circ}$ and $b$ = [-5.25, 5.25] $^{\circ}$

Yiwei Dong, Yan Sun, Ye Xu +11

We present the results of an unbiased $^{12}$ CO/ $^{13}$ CO/C $^{18}$ O ( $J$ = 1-0) survey in a portion of the third Galactic quadrant (TGQ): $l$ = [219.75, 229.75] $^{\circ}$ and $b$ = […

Kinematics of Young Stellar Objects Under Various Stellar Feedback

Molecular Bubble and Outflow in S Mon Revealed by Multiband Datasets

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

Distributions and Physical Properties of Molecular Clouds in the Third Galactic Quadrant: $l$ = [219.75, 229.75] $^{\circ}$ and $b$ = [-5.25, 5.25] $^{\circ}$