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Protostellar Outflow Heating in a Growing Massive Protocluster
Ke Wang, Qizhou Zhang, Yuefang Wu +2
The dense molecular clump P1 in the infrared dark cloud (IRDC) complex G28.34+0.06 harbors a massive protostellar cluster at its extreme youth. Our previous Submillimeter Array (SM…
The Origin of OB Clusters: From 10 pc to 0.1 pc
Hauyu Baobab Liu, Guillermo Quintana-Lacaci, Ke Wang +4
We observe the 1.2 mm continuum emission around the OB cluster forming region G10.6-0.4, using the IRAM 30m telescope MAMBO-2 bolometer array and the Submillimeter array. Compariso…
Hierarchical Fragmentation and Jet-like Outflows in IRDC G28.34+0.06, a Growing Massive Protostar Cluster
Ke Wang, Qizhou Zhang, Yuefang Wu +1
We present Submillimeter Array (SMA) λ= 0.88mm observations of an infrared dark cloud (IRDC) G28.34+0.06. Located in the quiescent southern part of the G28.34 cloud, the region of…
IRDC G030.88+00.13: A Tale of Two Massive Clumps
Qizhou Zhang, Ke Wang
Massive stars (M $\gsim 10$ \msun) form from collapse of parsec-scale molecular clumps. How molecular clumps fragment to give rise to massive stars in a cluster with a distribution…