activity
20162022
most citedOn the reservoir of sulphur in dark clouds : chemistry and elemental abundance reconciled

222 citations · 772 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2022★ 6 cited

Confirmation of the outflow in L1451-mm: SiO line and CHOH maser detections

V. Wakelam, A. Coutens, P. Gratier +2

The observational counterparts of theoretically predicted first hydrostatic cores (FHSC) have been searched for in the interstellar medium for nearly two decades now. Distinguishin…

astro-ph.GA2019★ 2 cited

New constraints on the initial parameters of low-mass star formation from chemical modeling

Thomas H. G. Vidal, Pierre Gratier, Neil Vaytet +2

The complexity of physico-chemical models of star formation is increasing, with models that take into account new processes and more realistic setups. These models allow astrochemi…

astro-ph.GA2018★ 29 cited

Methyl cyanide (CH3CN) and propyne (CH3CCH) in the low mass protostar IRAS 16293-2422

Ines Andron, Pierre Gratier, Liton Majumdar +4

Methyl cyanide (CH3CN) and propyne (CH3CCH) are two molecules commonly used as gas thermometers for interstellar gas. They are detected in several astrophysical environments and in…

astro-ph.GA2018★ 128 cited

Gas phase Elemental abundances in Molecular cloudS (GEMS) I. The prototypical dark cloud TMC 1

A. Fuente, D. Navarro, P. Caselli +30

GEMS is an IRAM 30m Large Program whose aim is determining the elemental depletions and the ionization fraction in a set of prototypical star-forming regions. This paper presents t…

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.GA2017★ 78 cited

First detection of interstellar S2H

Asunción Fuente, Javier R. Goicoechea, Jerome Pety +11

We present the first detection of gas phase S2H in the Horsehead, a moderately UV-irradiated nebula. This confirms the presence of doubly sulfuretted species in the interstellar me…