activity
20152024
most citedConstraining mixing in massive stars in the Small Magellanic Cloud

130 citations · 823 across the 26 of their papers we have counts for

collaborators

26 papers

astro-ph.GA2024

Revisiting the Velocity Dispersion-Size Relation in Molecular Cloud Structures

Haoran Feng, Zhiwei Chen, Zhibo Jiang +10

Structures in molecular ISM are observed to follow a power-law relation between the velocity dispersion and spatial size, known as Larson's first relation, which is often attribute…

astro-ph.GA2024★ 3 cited

On the Flux-Intensity Relation of Molecular Clouds

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

In this work, we report a study on the relationship between flux and intensity for molecular clouds. Our analysis is established on high-quality CO images from the Milky Way Imagin…

astro-ph.GA2023

The molecular clouds in a section of the third Galactic quadrant: observational properties and chemical abundance ratio between CO and its isotopologues

Chen Wang, Haoran Feng, Ji Yang +6

We compare the observational properties between CO, CO, and CO and summarize the observational parameters based on 7069 clouds sample from the Milky Way Imagin…

astro-ph.GA2023★ 3 cited

Updated Inventory of Carbon Monoxide in The Taurus Molecular Cloud

Yan Duan, Di Li, Laurent Pagani +4

The most extensive survey of carbon monoxide (CO) gas in the Taurus molecular cloud relied on CO and CO emission only, distinguishing the region w…

astro-ph.SR2022★ 24 cited

The initial spin distribution of B-type stars revealed by the split main sequences of young star clusters

Chen Wang, Ben Hastings, Abel Schootemeijer +6

Spectroscopic observations of stars in young open clusters have revealed evidence for a dichotomous distribution of stellar rotational velocities, with 10-30% of stars rotating slo…

astro-ph.GA2022★ 5 cited

Discovery of a New Molecular Bubble-Outflow Structure in the Taurus B18 Cloud

Yan Duan, Di Li, Paul F. Goldsmith +5

Star formation can produce bubbles and outflows, as a result of stellar feedback. Outflows and bubbles inject momentum and energy into the surrounding interstellar medium, and so a…