activity
20202026
most citedFormation of the Musca filament: Evidence for asymmetries in the accretion flow due to a cloud-cloud collision

50 citations · 50 across the 5 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

5 papers · 1 filter

astro-ph.GA2026

Molecular cloud dispersal traced by the ionized carbon 158 micron line

L. Bonne, N. Schneider, S. Dannhauer +14

Feedback from massive stars in the form of radiation and winds impacts the associated host molecular cloud. Feedback can disperse cloud material and lead to the destruction of the…

astro-ph.GA2026

CII fine-structure line observations of the Sagittarius C Region in the Galaxy's Central Molecular Zone

DEnise Riquelme-Vasquez, Rolf Guesten, Mark R. Morris +7

Context. Sagittarius C (Sgr C) is a massive, relatively quiescent complex at the western edge of the Galaxy's Central Molecular Zone (CMZ). While the Sgr B2 region has been extensi…

astro-ph.GA2025

Faint absorption of the ground state hyperfine-splitting transitions of hydroxyl at 18 cm in the Galactic Disk

M. R. Rugel, H. Beuther, J. D. Soler +15

The interstellar hydride hydroxyl (OH) is a potential tracer of CO-dark molecular gas. We present new absorption line observations of OH at 18-cm wavelength towards four continuum…

astro-ph.GA2024

Kinematics Star Formation in the Hub-Filament System G6.55-0.1

Saurav Sen, Bhaswati Mookerjea, Rolf Guesten +2

Hub-filament systems (HFSs) being the potential sites of formation of star clusters and high mass stars, provide a test bed for the current theories that attempt to explain star fo…

astro-ph.GA2020★ 50 cited

Formation of the Musca filament: Evidence for asymmetries in the accretion flow due to a cloud-cloud collision

L. Bonne, S. Bontemps, N. Schneider +11

Context. Dense molecular filaments are ubiquituous in the interstellar medium, yet their internal physical conditions and formation mechanism remain debated. Aims. We study the kin…