activity
20172026
most citedThe Green Bank Ammonia Survey (GAS): First Results of NH3 mapping the Gould Belt

159 citations · 926 across the 24 of their papers we have counts for

collaborators

25 papers

astro-ph.GA2026

Cracking open the "dragon egg": ALMA 1.3mm observations of a compact, young high-mass core candidate at 30mas resolution

A. T. Barnes, J. D. Henshaw, Á. Sánchez-Monge +14

Massive prestellar cores are a central assumption of core-accretion models of high-mass star formation, yet convincing observational examples remain rare. The "dragon egg" (C2c1a)…

astro-ph.GA2023★ 14 cited

Nitrogen fractionation in ammonia and its insights on nitrogen chemistry

Elena Redaelli, Luca Bizzocchi, Paola Caselli +1

Context. Observations of in the interstellar medium are becoming more frequent thanks to the increased telescope capabilities. However, interpreting these data…

astro-ph.GA2023★ 33 cited

First ALMA maps of cosmic ray ionisation rate in high-mass star-forming regions

Giovanni Sabatini, Stefano Bovino, Elena Redaelli

Low-energy cosmic rays ( TeV) are a pivotal source of ionisation of the interstellar medium, where they play a central role in determining the gas chemical composition and dras…

astro-ph.GA2023★ 2 cited

The kinematics of the magnetised protostellar core IRAS15398-3359

Farideh. S. Tabatabaei, Elena Redaelli, Paola Caselli +1

Observations of protostellar envelopes are essential to understand better the process of gravitational collapse toward star and planet formation. From a theoretical perspective, ma…

astro-ph.GA2022★ 17 cited

A large (~1 pc) contracting envelope around the prestellar core L1544

E. Redaelli, A. Chacón-Tanarro, P. Caselli +4

Prestellar cores, the birthplace of Sun-like stars, form from the fragmentation of the filamentary structure that composes molecular clouds, from which they must inherit at least p…

astro-ph.GA2022★ 38 cited

The core population and kinematics of a massive clump at early stages: an ALMA view

E. Redaelli, S. Bovino, P. Sanhueza +5

High-mass star formation theories make distinct predictions on the properties of the prestellar seeds of high-mass stars. Observations of the early stages of high-mass star formati…