55 citations · 171 across the 7 of their papers we have counts for
7 papers
Opacities of dense gas tracers in galactic massive star-forming regions
Shu Liu, Junzhi Wang, Fei Li +5
Optical depths of dense molecular gas are commonly used in Galactic and extragalactic studies to constrain the dense gas mass of the clouds or galaxies. The optical depths are ofte…
Abundance ratios of OH/CO and HCO+/CO as probes of the cosmic ray ionization rate in diffuse clouds
Gan Luo, Zhiyu Zhang, Thomas G. Bisbas +6
The cosmic-ray ionization rate (CRIR, ) is one of the key parameters controlling the formation and destruction of various molecules in molecular clouds. However, the current m…
Near-infrared chemical abundances of stars in the Sculptor dwarf galaxy
Baitian Tang, Jiajun Zhang, Zhiqiang Yan +3
Owing to the recent identification of major substructures in our Milky Way (MW), the astronomical community has started to reevaluate the importance of dissolved and existing dwarf…
First Data Release of the ESO-ARO Public Survey SAMPLING --- SMT "All-sky" Mapping of PLanck Interstellar Nebulae in the Galaxy
Ke Wang, Sarolta Zahorecz, Maria R. Cunningham +17
We make the first data release (DR1) of the ongoing ESO Public Survey SAMPLING (http://dx.doi.org/10.7910/DVN/0L8NHX). DR1 comprises of 124 fields distributed in $70^\circ < l < 21…
The Molecular Gas Environment in the 20 km s Cloud in the Central Molecular Zone
Xing Lu, Qizhou Zhang, Jens Kauffmann +9
We recently reported a population of protostellar candidates in the 20 km s cloud in the Central Molecular Zone of the Milky Way, traced by HO masers in gravitationally…
Cloud Structure of Galactic OB Cluster Forming Regions from Combining Ground and Space Based Bolometric Observations
Yuxin Lin, Hauyu Baobab Liu, Di Li +13
We have developed an iterative procedure to systematically combine the millimeter and submillimeter images of OB cluster-forming molecular clouds, which were taken by ground based…
Outflow detection in a 70 m dark high-mass core
S. Feng, H. Beuther, Q. Zhang +4
We present observations towards a high-mass (), low luminosity () m dark molecular core G 28.34 S-A at 3.4 mm, using the IRAM 30…