activity
19942026
most citedA computer program for fast non-LTE analysis of interstellar line spectra

1.7k citations · 41.8k across the 478 of their papers we have counts for

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Showing 2010 · astro-ph.GAShow all

14 papers · 2 filters

astro-ph.GA2010★ 262 cited

Water in Star-Forming Regions with the Herschel Space Observatory (WISH): Overview of key program and first results

E. F. van Dishoeck, L. E. Kristensen, A. O. Benz +12

`Water In Star-forming regions with Herschel' (WISH) is a key program on the Herschel Space Observatory designed to probe the physical and chemical structure of young stellar objec…

astro-ph.GA2010★ 33 cited

Variations in H2O+/H2O ratios toward massive star-forming regions

F. Wyrowski, F. van der Tak, F. Herpin +63

Early results from the Herschel Space Observatory revealed the water cation H2O+ to be an abundant ingredient of the interstellar medium. Here we present new observations of the H2…

astro-ph.GA2010★ 24 cited

Water abundances in high-mass protostellar envelopes: Herschel observations with HIFI

M. Marseille, F. F. S. van der Tak, F. Herpin +4

We derive the dense core structure and the water abundance in four massive star-forming regions which may help understand the earliest stages of massive star formation. We present…

astro-ph.GA2010★ 101 cited

Hydrides in Young Stellar Objects: Radiation tracers in a protostar-disk-outflow system

Arnold O. Benz, Simon Bruderer, Ewine F. van Dishoeck +2

Context: Hydrides of the most abundant heavier elements are fundamental molecules in cosmic chemistry. Some of them trace gas irradiated by UV or X-rays. Aims: We explore the abund…

astro-ph.GA2010★ 101 cited

Herschel/HIFI discovery of interstellar chloronium (HCl)

D. C. Lis, J. C. Pearson, D. A. Neufeld +102

We report the first detection of chloronium, HCl, in the interstellar medium, using the HIFI instrument aboard the \emph{Herschel} Space Observatory. The li…

astro-ph.GA2010★ 53 cited

Water vapor toward starless cores: the Herschel view

P. Caselli, E. Keto, L. Pagani +63

SWAS and Odin provided stringent upper limits on the gas phase water abundance of dark clouds (x(H2O) < 7x10^-9). We investigate the chemistry of water vapor in starless cores beyo…