activity
20062023
most citedWater in Star-Forming Regions with the Herschel Space Observatory (WISH): Overview of key program and first results

262 citations · 1k across the 19 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

11 papers · 1 filter

astro-ph.GA2023★ 19 cited

HCN emission from translucent gas and UV-illuminated cloud edges revealed by wide-field IRAM 30m maps of Orion B GMC: Revisiting its role as tracer of the dense gas reservoir for star formation

M. G. Santa-Maria, J. R. Goicoechea, J. Pety +28

We present 5 deg^2 (~250 pc^2) HCN, HNC, HCO+, and CO J=1-0 maps of the Orion B GMC, complemented with existing wide-field [CI] 492 GHz maps, as well as new pointed observations of…

astro-ph.GA2015★ 23 cited

Stratified NH and ND emission in the prestellar core 16293E in L1689N

A. Bacmann, F. Daniel, P. Caselli +6

High degrees of deuterium fractionation are commonly found in cold prestellar cores and in the envelopes around young protostars. As it brings strong constraints to chemical models…

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★ 77 cited

Nitrogen hydrides in the cold envelope of IRAS16293-2422

Pierre Hily-Blant, Sébastien Maret, Aurore Bacmann +4

Nitrogen is the fifth most abundant element in the Universe, yet the gas-phase chemistry of N-bearing species remains poorly understood. Nitrogen hydrides are key molecules of nitr…

astro-ph.GA2010★ 16 cited

Herschel/HIFI observations of spectrally resolved methylidyne signatures toward the high-mass star-forming core NGC6334I

M. H. D. van der Wiel, F. F. S. van der Tak, D. C. Lis +65

In contrast to extensively studied dense star-forming cores, little is known about diffuse gas surrounding star-forming regions. We study molecular gas in the high-mass star-formin…

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★ 36 cited

Herschel observations of extra-ordinary sources: Detecting spiral arm clouds by CH absorption lines

S. -L. Qin, P. Schilke, C. Comito +67

We have observed CH absorption lines () against the continuum source Sgr~B2(M) using the \textit{Herschel}/HIFI instrument. With the high spectral…

astro-ph.GA2010★ 57 cited

Herschel/HIFI measurements of the ortho/para ratio in water towards Sagittarius B2(M) and W31C

D. C. Lis, T. G. Phillips, P. F. Goldsmith +74

We present Herschel/HIFI observations of the fundamental rotational transitions of ortho- and para-HO and HO in absorption towards Sagittarius~B2(M) and W31C. The…

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…

astro-ph.GA2010★ 37 cited

Water abundance variations around high-mass protostars: Herschel-HIFI observations of the DR21 region

F. F. S. van der Tak, M. G. Marseille, F. Herpin +1

Water is a key molecule in the star formation process, but its spatial distribution in star-forming regions is not well known. We study the distribution of dust continuum and H2O a…