activity
20042008
most citedSMA Imaging of CO(3-2) Line and 860 micron Continuum of Arp 220 : Tracing the Spatial Distribution of Luminosity

139 citations · 863 across the 12 of their papers we have counts for

collaborators

16 papers

astro-ph2008104 cited

Spitzer IRAC and MIPS Imaging of Clusters and Outflows in 9 High-mass Star Forming Regions

Keping Qiu, Qizhou Zhang, S. Thomas Megeath +6

We present Spitzer Space Telescope IRAC and MIPS observations toward a sample of nine high-mass star forming regions at a distance of around 2 kpc. Based on IRAC and MIPS 24 m p…

astro-ph2008139 cited

SMA Imaging of CO(3-2) Line and 860 micron Continuum of Arp 220 : Tracing the Spatial Distribution of Luminosity

Kazushi Sakamoto, Junzhi Wang, Martina C. Wiedner +6

We used the Submillimeter Array (SMA) to image 860 micron continuum and CO(3-2) line emission in the ultraluminous merging galaxy Arp 220, achieving a resolution of 0.23" (80 pc) f…

astro-ph200725 cited

An evolved disk surrounding the massive main sequence star MWC 297?

P. Manoj, Paul T. P. Ho, Nagayoshi Ohashi +5

We present the results of the interferometric observations of the circumstellar disk surrounding MWC 297 in the continuum at 230 GHz (1.3 mm) and in the (J=2-1) rotational transiti…

astro-ph200792 cited

Submillimeter arcsecond-resolution mapping of the highly collimated protostellar jet HH 211

Chin-Fei Lee, Paul T. P. Ho, Aina Palau +4

We have mapped the protostellar jet HH 211 in 342 GHz continuum, SiO (), and CO () emission at \arcs{1} resolution with the Submillimeter Array (SMA). Thermal…

astro-ph2007112 cited

The Early Evolution of Massive Stars: Radio Recombination Line Spectra

Eric Keto, Qizhou Zhang, Stanley Kurtz

Velocity shifts and differential broadening of radio recombination lines are used to estimate the densities and velocities of the ionized gas in several hypercompact and ultracompa…

astro-ph200755 cited

A Jet-like Outflow toward the High-Mass (Proto)stellar Object IRAS 18566+0408

Qizhou Zhang, T. K. Sridharan, Todd R. Hunter +3

We performed interferometric observations of a high-mass protostellar candidate IRAS 18566+0408 in the \nh3 (J,K)=(1,1), (2,2) and (3,3) inversion transitions, the SiO J=2-1 and HC…