activity
20192022
most citedEdge collapse and subsequent longitudinal accretion in Filament S242

27 citations · 57 across the 5 of their papers we have counts for

collaborators

8 papers

astro-ph.GA20227 cited

CO Emission Delineating the Interface between the Milky Way Nuclear Wind Cavity and the Gaseous Disk

Yang Su, Shiyu Zhang, Ji Yang +8

Based on the MWISP survey, we study high-z CO emission toward the tangent points, in which the distances of the molecular clouds (MCs) are well determined. In the region of l=12-26…

astro-ph.GA202113 cited

A wide-field CO survey towards the California Molecular Filament

Weihua Guo, Xuepeng Chen, Jiancheng Feng +9

We present the survey of CO/CO/CO (J=1-0) toward the California Molecular Cloud (CMC) within the region of 161.75 167.75$^{\cir…

astro-ph.GA2021

A search for cloud cores affected by shocked carbon chain chemistry in L1251

Xunchuan Liu, Y. Wu, C. Zhang +26

We searched for shocked carbon chain chemistry (SCCC) sources with CS abundances surpassing those of HCN towards the dark cloud L1251, using the Effelsberg telescope at K-b…

astro-ph.GA2020

Planck Galactic Cold Clumps in Two Regions: the First Quadrant and the Anti-Center Direction Region

Chao Zhang, Yuefang Wu, Xunchuan Liu +13

Sixty five Planck Galactic cold clumps (PGCCs) from the first quadrant (IQuad) and thirty nine of PGCCs from the Anti-Center direction region (ACent) were observed in CO, $^…

astro-ph.GA202027 cited

Edge collapse and subsequent longitudinal accretion in Filament S242

Lixia Yuan, Guang-Xing Li, Ming Zhu +7

Filament S242 is 25 pc long with massive clumps and YSO clusters concentrated in its end regions; it is considered a good example of edge collapse. We mapped this filament in the $…

astro-ph.GA2019

Using CO line ratios to trace compressed areas in bubble N131

Chuan-Peng Zhang, Guang-Xing Li, Chenlin Zhou +2

N131 is a typical infrared dust bubble showing an expanding ringlike shell. We study what kinds of CO line ratios can be used to trace the interaction in the expanding bubble. We c…