activity
20172026
most citedDiscovery in space of ethanolamine, the simplest phospholipid head group

128 citations · 1.3k across the 99 of their papers we have counts for

collaborators
Showing 2022Show all

12 papers · 1 filter

astro-ph.GA2022★ 17 cited

CHEMOUT: CHEMical complexity in star-forming regions of the OUTer Galaxy III. Nitrogen isotopic ratios in the outer Galaxy

L. Colzi, D. Romano, F. Fontani +6

Nitrogen isotopic ratios are a key tool for tracing Galactic stellar nucleosynthesis. We present the first study of the N/N abundance ratio in the outer regions of th…

astro-ph.GA2022★ 43 cited

Tracing Interstellar Heating: An ALCHEMI Measurement of the HCN Isomers in NGC 253

Erica Behrens, Jeffrey G. Mangum, Jonathan Holdship +17

We analyze HCN and HNC emission in the nearby starburst galaxy NGC 253 to investigate its effectiveness in tracing heating processes associated with star formation. This study uses…

astro-ph.GA2022★ 18 cited

ALCHEMI finds a "shocking" carbon footprint in the starburst galaxy NGC~253

Nanase Harada, Sergio Martin, Jeff Mangum +15

Centers of starburst galaxies may be characterized by a specific gas and ice chemistry due to their gas dynamics and the presence of various ice desorption mechanisms. This may res…

astro-ph.GA2022★ 1 cited

Molecular precursors of the RNA-world in space: new nitriles in the G+0.693-0.027 molecular cloud

Víctor M. Rivilla, Izaskun Jiménez-Serra, Jesus Martín-Pintado +10

Nitriles play a key role as molecular precursors in prebiotic experiments based on the RNA-world scenario for the origin of life. These chemical compounds could have been partially…

astro-ph.GA2022★ 12 cited

CHEMOUT: CHEMical complexity in star-forming regions of the OUTer Galaxy. II. Methanol formation at low metallicity

F. Fontani, A. Schmiedeke, A. Sanchez-Monge +8

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

astro-ph.GA2022★ 32 cited

Energizing Star Formation: The Cosmic Ray Ionization Rate in NGC 253 Derived From ALCHEMI Measurements of HO and SO

Jonathan Holdship, Jeffrey G. Mangum, Serena Viti +16

The cosmic ray ionization rate (CRIR) is a key parameter in understanding the physical and chemical processes in the interstellar medium. Cosmic rays are a significant source of en…