activity
20152019
most citedSulphur chemistry in the L1544 pre-stellar core

140 citations · 593 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.SR2019★ 23 cited

On the nature of the compact sources in IRAS 16293-2422 seen in at centimeter to sub-millimeter wavelengths

Antonio Hernández-Gómez, Laurent Loinard, Claire J. Chandler +10

We present multi-epoch continuum observations of the Class 0 protostellar system IRAS 16293-2422 taken with the Very Large Array (VLA) at multiple wavelengths between 7 mm and 15 c…

astro-ph.GA2019★ 78 cited

First detection of the pre-biotic molecule glycolonitrile (HOCH2CN) in the interstellar medium

S. Zeng, D. Quénard, I. Jiménez-Serra +4

Theories of a pre-RNA world suggest that glycolonitrile (HOCHCN) is a key species in the process of ribonucleotide assembly, which is considered as a molecular precursor of nuc…

astro-ph.GA2018★ 11 cited

The fate of formamide in a fragmenting protoplanetary disc

David Quénard, John D. Ilee, Izaskun Jiménez-Serra +3

Recent high-sensitivity observations carried out with ALMA have revealed the presence of complex organic molecules (COMs) such as methyl cyanide (CHCN) and methanol (CH$_…

astro-ph.GA2018★ 140 cited

Sulphur chemistry in the L1544 pre-stellar core

Charlotte Vastel, David Quénard, Romane Le Gal +7

The L1544 pre-stellar core has been observed as part of the ASAI IRAM 30m Large Program as well as follow-up programs. These observations have revealed the chemical richness of the…

astro-ph.SR2017★ 32 cited

Chemical modelling of glycolaldehyde and ethylene glycol in star-forming regions

A. Coutens, S. Viti, J. M. C. Rawlings +5

Glycolaldehyde (HOCHCHO) and ethylene glycol ((CHOH)) are two complex organic molecules detected in the hot cores and hot corinos of several star-forming regions. The e…

astro-ph.GA2017★ 79 cited

Phosphorus-bearing molecules in the Galactic Center

V. M. Rivilla, I. Jiménez-Serra, S. Zeng +10

Phosphorus (P) is one of the essential elements for life due to its central role in biochemical processes. Recent searches have shown that P-bearing molecules (in particular PN and…

astro-ph.GA2017★ 25 cited

High spectral resolution observations of HNC3 and HCCNC in the L1544 prestellar core

C. Vastel, K. Kawaguchi, D. Quénard +4

HCCNC and HNC3 are less commonly found isomers of cyanoacetylene, HC3N, a molecule that is widely found in diverse astronomical sources. We want to know if HNC3 is present in sourc…

astro-ph.SR2017★ 108 cited

Chemical modelling of complex organic molecules with peptide-like bonds in star-forming regions

David Quénard, Izaskun Jiménez-Serra, Serena Viti +2

Peptide bonds (N-C=O) play a key role in metabolic processes since they link amino acids into peptide chains or proteins. Recently, several molecules containing peptide-like bonds…

astro-ph.GA2017★ 35 cited

The ALMA Frontier Fields Survey - II. Multiwavelength Photometric analysis of 1.1mm continuum sources in Abell 2744, MACSJ0416.1-2403 and MACSJ1149.5+2223

N. Laporte, F. E. Bauer, P. Troncoso-Iribarren +32

[abridged] The Hubble and Spitzer Space Telescope surveys of the Frontier Fields (FF) provide extremely deep images around six massive, strong-lensing clusters of galaxies. The ALM…

astro-ph.GA2017★ 47 cited

Detection of the HCNH and HCNH ions in the L1544 pre-stellar core

David Quénard, Charlotte Vastel, Cecilia Ceccarelli +3

The L1544 pre-stellar core was observed as part of the ASAI (Astrochemical Surveys At IRAM) Large Program. We report the first detection in a pre-stellar core of the HCNH and H…

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.SR2015★ 7 cited

Detectability of deuterated water in prestellar cores

David Quénard, Vianney Taquet, Charlotte Vastel +2

Water is an important molecule in the chemical and thermal balance of dense molecular gas, but knowing its history through-out the various stages of the star formation is a fundame…