activity
20162022
most citedThe Milky Way Imaging Scroll Painting (MWISP): Project Details and Initial Results from the Galactic Longitude of 25.8deg to 49.7deg

203 citations · 360 across the 12 of their papers we have counts for

collaborators

16 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

Examinations of CO completeness based on three independent CO surveys

Yan Sun, Ji Yang, Qing-Zeng Yan +7

We report the global properties recovered by an ongoing CO survey of the Milky Way Imaging Scroll Painting (MWISP) toward the Galactic outskirts. %To better understand the observat…

astro-ph.GA2021

High-resolution CARMA Observation of Molecular Gas in the North America and Pelican Nebulae

Shuo Kong, Héctor G. Arce, John M. Carpenter +15

We present the first results from a CARMA high-resolution CO(1-0), CO(1-0), and CO(1-0) molecular line survey of the North America and Pelican (NAP) Nebulae. C…

astro-ph.GA202129 cited

Molecular gas distribution perpendicular to the Galactic plane

Yang Su, Ji Yang, Qing-Zeng Yan +9

We use the ~370 square degrees data from the MWISP CO survey to study the vertical distribution of the molecular clouds (MCs) toward the tangent points in the region of l=[16,52]de…

astro-ph.GA2020

Testing the star formation scaling relations in the clumps of the North American and Pelican cloud complexes

Swagat R. Das, Jessy Jose, Manash R Samal +2

The processes which regulate the star-formation within molecular clouds are still not well understood. Various star-formation scaling relations have been proposed to explain this i…