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20102015
most citedWater in Star-Forming Regions with the Herschel Space Observatory (WISH): Overview of key program and first results

262 citations · 2.2k across the 28 of their papers we have counts for

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23 papers · 1 filter

astro-ph.GA2015★ 15 cited

Rotational spectra of isotopic species of methyl cyanide, CHCN, in their excited vibrational states

H. S. P. Müller, B. J. Drouin, J. C. Pearson +3

Methyl cyanide is an important trace molecule in space, especially in star-forming regions where it is one of the more common molecules used to derive kinetic temperatures. We want…

astro-ph.GA2014★ 149 cited

Ubiquitous argonium (ArH) in the diffuse interstellar medium -- a molecular tracer of almost purely atomic gas

Peter Schilke, David A. Neufeld, Holger S. P. Müller +14

We describe the assignment of a previously unidentified interstellar absorption line to ArH and discuss its relevance in the context of hydride absorption in diffuse gas with a…

astro-ph.GA2014★ 25 cited

Widespread Rotationally-Hot Hydronium Ion in the Galactic Interstellar Medium

D. C. Lis, P. Schilke, E. A. Bergin +11

We present new observations of the (6,6) and (9,9) inversion transitions of the hydronium ion toward Sagittarius B2(N) and W31C. Sensitive observations toward Sagittarius B2(N) sho…

astro-ph.GA2013★ 62 cited

Detection of the Ammonium Ion in Space

J. Cernicharo, B. Tercero, A. Fuente +9

We report on the detection of a narrow feature at 262816.73 MHz towards Orion and the cold prestellar core B1-bS, that we attribute to the 1(0)-0(0) line of the deuterated Ammonium…

astro-ph.GA2012★ 82 cited

Nitrogen hydrides in interstellar gas II. Analysis of Herschel/HIFI observations towards W49N and G10.6-0.4 (W31C)

C. M. Persson, M. De Luca, B. Mookerjea +14

We have used the Herschel-HIFI instrument to observe interstellar nitrogen hydrides along the sight-lines towards W49N and G10.6-0.4 in order to elucidate the production pathways l…

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★ 37 cited

Herschel observations of EXtra-Ordinary Sources (HEXOS): Observations of H2O and its isotopologues towards Orion KL

G. J. Melnick, V. Tolls, D. A. Neufeld +49

We report the detection of more than 48 velocity-resolved ground rotational state transitions of H2(16)O, H2(18)O, and H2(17)O - most for the first time - in both emission and abso…

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★ 35 cited

The distribution of water in the high-mass star-forming region NGC 6334I

M. Emprechtinger, D. C. Lis, T. Bell +66

We present observations of twelve rotational transitions of H2O-16, H2O-18, and H2O-17 toward the massive star-forming region NGC 6334 I, carried out with Herschel/HIFI as part of…

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★ 83 cited

Nitrogen hydrides in interstellar gas: Herschel/HIFI observations towards G10.6-0.4 (W31C)

C. M. Persson, J. H. Black, J. Cernicharo +49

The HIFI instrument on board the Herschel Space Observatory has been used to observe interstellar nitrogen hydrides along the sight-line towards G10.6-0.4 in order to improve our u…

astro-ph.GA2010★ 111 cited

Detection of hydrogen fluoride absorption in diffuse molecular clouds with Herschel/HIFI: a ubiquitous tracer of molecular gas

P. Sonnentrucker, D. A. Neufeld, T. G. Phillips +47

We discuss the detection of absorption by interstellar hydrogen fluoride (HF) along the sight line to the submillimeter continuum sources W49N and W51. We have used Herschel's HIFI…

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★ 51 cited

Strong CH+ J=1-0 emission and absorption in DR21

E. Falgarone, V. Ossenkopf, M. Gerin +30

We report the first detection of the ground-state rotational transition of the methylidyne cation CH+ towards the massive star-forming region DR21 with the HIFI instrument onboard…

astro-ph.GA2010★ 171 cited

Herschel/HIFI observations of interstellar OH+ and H2O+ towards W49N: a probe of diffuse clouds with a small molecular fraction

D. A. Neufeld, J. R. Goicoechea, P. Sonnentrucker +50

We report the detection of absorption by interstellar hydroxyl cations and water cations, along the sight-line to the bright continuum source W49N. We have used Herschel's HIFI ins…

astro-ph.GA2010★ 42 cited

Herschel observations of ortho- and para-oxidaniumyl (H2O+) in spiral arm clouds toward Sgr B2(M)

P. Schilke, C. Comito, H. S. P. Mueller +55

H2O+ has been observed in its ortho- and para- states toward the massive star forming core Sgr B2(M), located close to the Galactic center. The observations show absorption in all…

astro-ph.GA2010★ 76 cited

CHESS, Chemical Herschel surveys of star forming regions:Peering into the protostellar shock L1157-B1

B. Lefloch, S. Cabrit, C. Codella +74

The outflow driven by the low-mass class 0 protostar L1157 is the prototype of the so-called chemically active outflows. The bright bowshock B1 in the southern outflow lobe is a pr…

astro-ph.GA2010★ 185 cited

Interstellar OH+, H2O+ and H3O+ along the sight-line to G10.6-0.4

Maryvonne Gerin, M. De Luca, John Black +50

We report the detection of absorption lines by the reactive ions OH+, H2O+ and H3O+ along the line of sight to the submillimeter continuum source G10.60.4 (W31C). We used the He…

astro-ph.GA2010★ 107 cited

Water cooling of shocks in protostellar outflows: Herschel-PACS map of L1157

B. Nisini, M. Benedettini, C. Codella +62

In the framework of the Water in Star-forming regions with Herschel (WISH) key program, maps in water lines of several outflows from young stars are being obtained, to study the wa…

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…

astro-ph.GA2010★ 107 cited

Strong absorption by interstellar hydrogen fluoride: Herschel/HIFI observations of the sight-line to G10.6-0.4 (W31C)

D. A. Neufeld, P. Sonnentrucker, T. G. Phillips +45

We report the detection of strong absorption by interstellar hydrogen fluoride along the sight-line to the submillimeter continuum source G10.6-0.4 (W31C). We have used Herschel's…

astro-ph.GA2010★ 87 cited

Detection of interstellar oxidaniumyl: abundant H2O+ towards the star-forming regions DR21, Sgr B2, and NGC6334

V. Ossenkopf, H. S. P. Müller, D. C. Lis +99

We identify a prominent absorption feature at 1115 GHz, detected in first HIFI spectra towards high-mass star-forming regions, and interpret its astrophysical origin. The character…