activity
20062008
most citedSMA Imaging of CO(3-2) Line and 860 micron Continuum of Arp 220 : Tracing the Spatial Distribution of Luminosity

139 citations · 470 across the 7 of their papers we have counts for

collaborators

7 papers

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-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-ph200832 cited

ATCA 3mm observations of NGC6334I and I(N): dense cores, outflows and an UCHII region

H. Beuther, A. J. Walsh, S. Thorwirth +4

Aims: Investigation of the dense gas, the outflows and the continuum emission from the massive twin cores NGC6334I and I(N) at high spatial resolution. Methods: We imaged the regio…

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-ph200752 cited

Multi-line (sub)millimetre observations of the high-mass proto cluster IRAS 05358+3543

S. Leurini, H. Beuther, P. Schilke +3

Since most high- and intermediate-mass protostars are at great distance and form in clusters, high linear resolution observations are needed to investigate their physical propertie…