activity
20072025
most citedProtostellar birth with ambipolar and ohmic diffusion

106 citations · 694 across the 19 of their papers we have counts for

collaborators

19 papers

astro-ph.GA2025★ 6 cited

Mapping Synthetic Observations to Prestellar Core Models: An Interpretable Machine Learning Approach

T. Grassi, M. Padovani, D. Galli +6

Observations of molecular lines are a key tool to determine the main physical properties of prestellar cores. However, not all the information is retained in the observational proc…

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…

cs.MS2020★ 7 cited

Scipp: Scientific data handling with labeled multi-dimensional arrays for C++ and Python

Simon Heybrock, Owen Arnold, Igor Gudich +2

Scipp is heavily inspired by the Python library xarray. It enriches raw NumPy-like multi-dimensional arrays of data by adding named dimensions and associated coordinates. Multiple…

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.GA2019★ 14 cited

The challenges of modelling microphysics: ambipolar diffusion, chemistry, and cosmic rays in MHD shocks

T. Grassi, M. Padovani, J. P. Ramsey +4

From molecular clouds to protoplanetary disks, non-ideal magnetic effects are important in many astrophysical environments. Indeed, in star and disk formation processes, it has bec…

astro-ph.SR2018★ 106 cited

Protostellar birth with ambipolar and ohmic diffusion

Neil Vaytet, Benoît Commerçon, Jacques Masson +2

The transport of angular momentum is capital during the formation of low-mass stars; too little removal and rotation ensures stellar densities are never reached, too much and the a…