88 citations · 422 across the 9 of their papers we have counts for
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NH3 Observations of the Infrared Dark Cloud G28.34+0.06
Y. Wang, Q. Zhang, T. Pillai +2
We present observations of the \nh3 (J,K) = (1,1) and (2,2) inversion transitions toward the infrared dark cloud G28.34+0.06, using the Very Large Array. Strong NH3 emission is fou…
Spectral Energy Distributions of High Mass Proto Stellar Objects - Evidence for High Accretion Rates
F. M. Fazal, T. K. Sridharan, K. Qiu +3
The spectral energy distributions (SEDs), spanning the mid-infrared to millimeter wavelengths, of a sample of 13 high-mass protostellar objects (HMPOs) were studied using a large a…
The 10^5Lsun High-Mass Protostellar Object IRAS23151+5912
H. Beuther, Q. Zhang, T. R. Hunter +2
While most sources above 10^5Lsun have already formed an Ultracompact HII region (UCHII), this is not necessarily the case for sources of lower luminosity. Characterizing sources i…
Dust and gas emission in the prototypical hot core G29.96-0.02 at sub-arcsecond resolution
H. Beuther, Q. Zhang, E. A. Bergin +3
Aiming at a better understand of the physical and chemical processes in the hot molecular core stage of high-mass star formation, we observed the prototypical hot core G29.96-0.02…
Submillimeter Array Observations of 321 GHz Water Maser Emission in Cepheus A
N. A. Patel, S. Curil, Q. Zhang +3
Using the Submillimeter Array (SMA) we have imaged for the first time the 321.226 GHz, 10_{29}-9_{36} ortho-H2O maser emission. This is also the first detection of this line in the…