activity
20042008
most citedNH3 Observations of the Infrared Dark Cloud G28.34+0.06

88 citations · 422 across the 9 of their papers we have counts for

collaborators

10 papers

astro-ph200852 cited

Chemical Diversity in High-Mass Star Formation

H. Beuther, Q. Zhang, E. A. Bergin +1

Massive star formation exhibits an extremely rich chemistry. However, not much evolutionary details are known yet, especially at high spatial resolution. Therefore, we synthesize p…

astro-ph200877 cited

SMA observations of Infrared Dark Clouds: A tale of two cores

J. M. Rathborne, J. M. Jackson, Q. Zhang +1

We present high-angular resolution sub-millimeter continuum images and molecular line spectra obtained with the SMA toward two massive cores that lie within Infrared Dark Clouds; o…

astro-ph200788 cited

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…

astro-ph200720 cited

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…

astro-ph200717 cited

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…

astro-ph200781 cited

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…