S. Bian

activity

20182026

most citedA comparison of the local spiral structure from Gaia DR2 and VLBI maser parallaxes

84 citations · 352 across the 19 of their papers we have counts for

collaborators

Showing 2023Show all

3 papers · 1 filter

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: $l$ = [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 $b$ = […

astro-ph.GA2023★ 45 cited

What Does the Milky Way Look Like?

Y. Xu, C. J. Hao, D. J. Liu +5

In spite of much work, the overall spiral structure morphology of the Milky Way remains somewhat uncertain. In the last two decades, accurate distance measurements have provided us…

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

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

What Does the Milky Way Look Like?

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