activity
20012008
most cited{Millimeter Multiplicity in NGC 6334 I and I(N)

114 citations · 335 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph2008★ 32 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-ph2007★ 37 cited

Kinematics of a hot massive accretion disk candidate

H. Beuther, A. Walsh

Characterizing rotation, infall and accretion disks around high-mass protostars is an important topic in massive star formation research. With the Australia Telescope Compact Array…

astro-ph2007★ 52 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…

astro-ph2007★ 57 cited

Hot ammonia in NGC6334I & I(N)

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

Aims: The massive twin cores NGC6334I and I(N) are in different evolutionary stages and hence ideal targets to study evolutionary variations within the same larger-scale environmen…

astro-ph2006★ 114 cited

{Millimeter Multiplicity in NGC 6334 I and I(N)

T. R. Hunter, C. L. Brogan, S. T. Megeath +3

Using the Submillimeter Array (SMA), we have imaged the 1.3 millimeter continuum emission at the center of the massive star-forming regions NGC 6334 I and I(N). In both regions, th…

astro-ph2005★ 39 cited

High-spatial-resolution observations of NH3 and CH3OH towards the massive twin cores NGC6334 I & I(N)

H. Beuther, S. Thorwirth, Q. Zhang +4

Molecular line observations of NH3 (J,K)=(1,1), (2,2) and CH3OH at 24.93GHz taken with the Australian Telescope Compact Array (ATCA) toward the massive twin cores NGC6334 I & I(N)…