most citedSOLIS II. Carbon-chain growth in the Solar-type protocluster OMC2-FIR4

90 citations · 523 across the 13 of their papers we have counts for

collaborators

12 papers

astro-ph.GA2017★ 90 cited

SOLIS II. Carbon-chain growth in the Solar-type protocluster OMC2-FIR4

F. Fontani, C. Ceccarelli, C. Favre +42

The interstellar delivery of carbon atoms locked into molecules might be one of the key ingredients for the emergence of life. Cyanopolyynes are carbon chains delimited at their tw…

astro-ph.SR2017★ 8 cited

Modelling the 3D physical structure of astrophysical sources with GASS

D. Quénard, S. Bottinelli, E. Caux

The era of interferometric observations leads to the need of a more and more precise description of physical structures and dynamics of star-forming regions, from pre-stellar cores…

astro-ph.GA2017★ 21 cited

A study of singly deuterated cyclopropenylidene c-C3HD in protostar IRAS 16293-2422

L. Majumdar, P. Gratier, I. Andron +2

Cyclic-C3HD (c-C3HD) is a singly deuterated isotopologue of c-C3H2, which is one of the most abundant and widespread molecules in our Galaxy. We observed IRAS 16293-2422 in the 3 m…

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★ 49 cited

First detection of ND in the solar-mass protostar IRAS16293-2422

A. Bacmann, E. Caux, P. Hily-Blant +64

In the past decade, much progress has been made in characterising the processes leading to the enhanced deuterium fractionation observed in the ISM and in particular in the cold, d…

astro-ph.SR2010★ 31 cited

Herschel observations of EXtra-Ordinary Sources: The Terahertz spectrum of Orion KL seen at high spectral resolution

N. R. Crockett, E. A. Bergin, S. Wang +60

We present the first high spectral resolution observations of Orion KL in the frequency ranges 1573.4 - 1702.8 GHz (band 6b) and 1788.4 - 1906.8 GHz (band 7b) obtained using the HI…

astro-ph.SR2010★ 34 cited

Herschel/HIFI deepens the circumstellar NH3 enigma

K. M. Menten, F. Wyrowski, J. Alcolea +23

Circumstellar envelopes (CSEs) of a variety of evolved stars have been found to contain ammonia (NH3) in amounts that exceed predictions from conventional chemical models by many o…

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.SR2010★ 35 cited

Herschel observations of the hydroxyl radical (OH) in young stellar objects

S. F. Wampfler, G. J. Herczeg, S. Bruderer +58

Water in Star-forming regions with Herschel (WISH) is a Herschel Key Program investigating the water chemistry in young stellar objects (YSOs) during protostellar evolution. Hydrox…

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.SR2010★ 69 cited

Water content and wind acceleration in the envelope around the oxygen-rich AGB star IK Tau as seen by Herschel/HIFI

L. Decin, K. Justtanont, E. De Beck +4

During their asymptotic giant branch, evolution low-mass stars lose a significant fraction of their mass through an intense wind, enriching the interstellar medium with products of…