activity
20002003
most citedChemistry as a probe of the structures and evolution of massive star forming regions

156 citations · 468 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph2003★ 146 cited

Sulphur chemistry in the envelopes of massive young stars

F. F. S. van der Tak, A. M. S. Boonman, R. Braakman +1

The sulphur chemistry in nine regions in the earliest stages of high-mass star formation is studied through single-dish submillimeter spectroscopy. The line profiles indicate that…

astro-ph2002

Sulphur chemistry in the envelopes of massive young stars

F. F. S. van der Tak, A. M. S. Boonman, R. Braakman +1

We present submillimeter observations of SO, SO2, H2S, H2CS, OCS, NS and HCS+ toward nine massive young stars. The outflow contributes ~50% to the SO and SO2 emission in 15-20'' be…

astro-ph2002★ 156 cited

Chemistry as a probe of the structures and evolution of massive star forming regions

S. D. Doty, E. F. van Dishoeck, F. F. S. van der Tak +1

We present detailed thermal and gas-phase chemical models for the envelope of the massive star-forming region AFGL 2591. Time- and space-dependent chemistry are used to study the p…

astro-ph2001★ 76 cited

Gas-phase H2O and CO2 toward massive protostars

A. M. S. Boonman, E. F. van Dishoeck, F. Lahuis +2

We present a study of gas-phase H2O and CO2 toward a sample of 14 massive protostars with the Short Wavelength Spectrometer (SWS) on board the Infrared Space Observatory (ISO). Mod…

astro-ph2001★ 73 cited

Highly abundant HCN in the inner hot envelope of GL 2591: probing the birth of a hot core?

A. M. S. Boonman, R. Stark, F. F. S. van der Tak +5

We present observations of the v2=0 and vibrationally excited v2=1 J=9-8 rotational lines of HCN at 797 GHz toward the deeply embedded massive young stellar object GL 2591, which p…

astro-ph2000★ 17 cited

Infrared Observations of Hot Gas and Cold Ice toward the Low Mass Protostar Elias 29

A. C. A. Boogert, A. G. G. M. Tielens, C. Ceccarelli +5

We have obtained the full 1-200 um spectrum of the low luminosity (36 Lsun) Class I protostar Elias 29 in the Rho Ophiuchi molecular cloud. It provides a unique opportunity to stud…