activity
20182020
most citedA SiO J = 5 - 4 Survey Toward Massive Star Formation Regions

38 citations · 77 across the 3 of their papers we have counts for

collaborators

7 papers

astro-ph.GA202011 cited

CO observations toward HI-rich Ultra Diffuse Galaxies

Junzhi Wang, Kai Yang, Zhi-Yu Zhang +5

We present CO observations toward a sample of six HI-rich Ultra-diffuse galaxies (UDGs) as well as one UDG (VLSB-A) in the Virgo Cluster with the IRAM 30-m telescope. CO 1-0 is mar…

astro-ph.GA2020

ALMA observations of NGC 6334S I: Forming massive stars and cluster in subsonic and transonic filamentary clouds

Shanghuo Li, Qizhou Zhang, Hauyu Baobab Liu +11

We present Atacama Large Millimeter/submillimeter Array (ALMA) and Karl G. Jansky Very Large Array (JVLA) observations of the massive infrared dark cloud NGC 6334S (also known as I…

astro-ph.GA2020

HCN 3-2 survey towards a sample of local galaxies

Fei Li, Junzhi Wang, Min Fang +4

We present observations of HCN 3-2 emissions towards 37 local galaxies using 10-m Submillimeter Telescope (SMT). HCN 3-2 emission is detected in 23 galaxies. The correlation of inf…

astro-ph.SR201928 cited

Mapping Observations of complex organic molecules around Sagittarius B2 with ARO 12m telescope

Juan Li, Junzhi Wang, Haihua Qiao +10

We performed high-sensitivity mapping observations of several complex organic molecules around Sagittarius B2 with ARO 12m telescope at 3-mm wavelength. Based on their spatial dist…

astro-ph.GA2019

Formation of Massive Protostellar Clusters -- Observations of Massive 70 m Dark Molecular Clouds

Shanghuo Li, Qizhou Zhang, Thushara Pillai +3

We present Submillimeter Array (SMA) observations of seven massive molecular clumps which are dark in the far-infrared for wavelengths up to 70 m. Our 1.3 mm continuum images re…

astro-ph.GA201938 cited

A SiO J = 5 - 4 Survey Toward Massive Star Formation Regions

Shanghuo Li, Junzhi Wang, Min Fang +6

We performed a survey in the SiO line toward a sample of 199 Galactic massive star-forming regions at different evolutionary stages with the SMT 10 m and CSO 10.4…