2 citations · 2 across the 5 of their papers we have counts for
4 papers · 1 filter
ALOHA IRDCs Molecular Line Follow-up: I. Gas properties and kinematics
Jinjin Xie, Yaoting Yan, Zhiyuan Ren +109
Infrared Dark Clouds are ideal sites for investigating the initial conditions of massive star and cluster formation. The A Lei Of the Habitat and Assembly of Infrared Dark Clouds (…
The factors that influence protostellar multiplicity II. Gas temperature and mass in Perseus with APEX
N. M. Murillo, C. M. Fuchs, D. Harsono +5
Protostellar multiplicity is a common outcome of the star formation process. To fully understand the formation and evolution of these systems, the physical parameters of the molecu…
JCMT 850 $\micron$ continuum observations of density structures in the G35 molecular complex
Xianjin Shen, Hong-Li Liu, Zhiyuan Ren +32
Filaments are believed to play a key role in high-mass star formation. We present a systematic study of the filaments and their hosting clumps in the G35 molecular complex using JC…
APEX-SEPIA660 Early Science: Gas at densities above cm towards OMC-1
A. Hacar, M. R. Hogerheijde, D. Harsono +12
Context. The star formation rates and stellar densities found in young massive clusters suggest that these stellar systems originate from gas at densities n(H) cm$^{-3}…