activity
20032024
most citedThe Spitzer ice legacy: Ice evolution from cores to protostars

570 citations · 4.6k across the 51 of their papers we have counts for

collaborators

49 papers

astro-ph.GA2024

Modelling carbon chain and complex organic molecules in the DR21(OH) clump

P. Freeman, S. Bottinelli, R. Plume +2

Star-forming regions host a large and evolving suite of molecular species. Molecular transition lines, particularly of complex molecules, can reveal the physical and dynamical envi…

astro-ph.GA2023★ 3 cited

Parsec scales of carbon chain and complex organic molecules in AFGL 2591 and IRAS 20126

P. Freeman, S. Bottinelli, R. Plume +3

(Abridged) There is a diverse chemical inventory in protostellar regions leading to the classification of extreme types of systems. Warm carbon chain chemistry sources, for one, ar…

astro-ph.SR2022★ 14 cited

Mass ejection and time variability in protostellar outflows: Cep E. SOLIS XVI

A. de A. Schutzer, P. R. Rivera-Ortiz, B. Lefloch +46

Protostellar jets are an important agent of star formation feedback, tightly connected with the mass-accretion process. The history of jet formation and mass-ejection provides cons…

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.SR2018★ 19 cited

Modelling the abundance structure of isocyanic acid (HNCO) toward the low-mass solar type protostar IRAS 16293-2422

Antonio Hernández-Gómez, Emna Sahnoun, Emmanuel Caux +5

Isocyanic acid (HNCO), the most stable of the simplest molecules containing the four main elements essential for organic chemistry, has been observed in several astrophysical envir…

astro-ph.SR2018★ 11 cited

3D modelling of HCO and its isotopologues in the low-mass proto-star IRAS162932422

D. Quénard, S. Bottinelli, E. Caux +1

Ions and electrons play an important role in various stages of the star formation process. By following the magnetic field of their environment and interacting with neutral species…