activity
20082024
most citedEvolutionary study of complex organic molecules in high-mass star-forming regions

71 citations · 247 across the 11 of their papers we have counts for

collaborators

14 papers

astro-ph.GA2023

The GUAPOS project: G31.41+0.31 Unbiased ALMA sPectral Observational Survey. IV. Phosphorus-bearing molecules and their relation with shock tracers

F. Fontani, C. Mininni, M. T. Beltrán +6

The astrochemistry of the important biogenic element phosphorus (P) is still poorly understood, but observational evidence indicates that P-bearing molecules are likely associated…

astro-ph.GA2023

Radio survey of the stellar population in the infrared dark cloud G14.225-0.506

Elena Díaz-Márquez, Roger Grau, Gemma Busquet +8

The IRDC G14.225-0.506 is associated with a network of filaments, which result in two different dense hubs, as well as with several signposts of star formation activity. The aim of…

astro-ph.GA202224 cited

Velocity structure of the 50 pc-long NGC 6334 filamentary cloud: Hints of multiple compressions and their impact on the cloud properties?

Doris Arzoumanian, Delphine Russeil, Annie Zavagno +8

[Abridged] The interstellar medium is observed to be organised in filamentary structures, as well as neutral (HI) and ionized (HII) bubbles. The expanding nature of these bubbles m…

astro-ph.GA2021

Herschel observations of extraordinary sources: Full Herschel/HIFI molecular line survey of Sagittarius B2(M)

T. Möller, P. Schilke, A. Schmiedeke +5

We present a full analysis of a broadband spectral line survey of Sagittarius B2 (Main), one of the most chemically rich regions in the Galaxy located within the giant molecular cl…

astro-ph.GA202138 cited

ALMA-IRDC: Dense gas mass distribution from cloud to core scales

A. T. Barnes, J. D. Henshaw, F. Fontani +15

Infrared dark clouds (IRDCs) are potential hosts of the elusive early phases of high-mass star formation (HMSF). Here we conduct an in-depth analysis of the fragmentation propertie…

astro-ph.GA202119 cited

Fragmentation in the massive G31.41+0.31 protocluster

M. T. Beltrán, V. M. Rivilla, R. Cesaroni +18

Context. ALMA observations at 1.4 mm and 0.2'' (750au) angular resolution of the Main core in the high-mass star forming region G31.41+0.31 have revealed a puzzling scenario: on th…