activity
20182022
most citedThe GUAPOS project II. A comprehensive study of peptide-like bond molecules

55 citations · 99 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.GA202219 cited

CHEMOUT: CHEMical complexity in star-forming regions of the OUTer Galaxy. I. Organic molecules and tracers of star-formation activity

F. Fontani, L. Colzi, L. Bizzocchi +8

The outer Galaxy is an environment with metallicity lower than the Solar one. Because of this, the formation and survival of molecules in star-forming regions located in the inner…

astro-ph.GA202112 cited

Probing the kinematics and chemistry of the hot core Mon R 2 IRS 3 using ALMA observations

A. Fuente, S. P. Treviño-Morales, T. Alonso-Albi +3

We present high angular resolution 1.1mm continuum and spectroscopic ALMA observations of the well-known massive proto-cluster Mon R 2 IRS 3.The continuum image at 1.1mm shows two…

astro-ph.GA202155 cited

The GUAPOS project II. A comprehensive study of peptide-like bond molecules

L. Colzi, V. M. Rivilla, M. T. Beltrán +12

Peptide-like bond molecules, which can take part to the formation of proteins in a primitive Earth environment, have been detected up to now only towards a few sources. We present…

astro-ph.GA202113 cited

The TOPGöt high-mass star-forming sample. I. Methyl cyanide emission as tracer of early phases of star formation

C. Mininni, F. Fontani, A. Sánchez-Monge +9

The TOPGöt project studies a sample of 86 high-mass star-forming regions in different evolutionary stages from starless cores to ultra compact HII regions. The aim of the survey is…

astro-ph.SR2018

Nitrogen fractionation in high-mass star-forming cores across the Galaxy

L. Colzi, F. Fontani, V. M. Rivilla +4

The fractionation of nitrogen (N) in star-forming regions is a poorly understood process. To put more stringent observational constraints on the N-fractionation, we have observed w…

astro-ph.GA2018

The fragmentation properties of massive protocluster gas clumps: an ALMA study

F. Fontani, B. Commerçon, A. Giannetti +5

Fragmentation of massive dense molecular clouds is the starting point in the formation of rich clusters and massive stars. Theory and numerical simulations indicate that the popula…