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20212026
most citedMulti-scale view of star formation in IRAS 21078+5211: From clump fragmentation to disk wind

28 citations · 53 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2026

The CepA disk-outflow system at <=0.2'' or <=100au resolution

H. Beuther, C. Gieser, V. Aberham +21

Context: Although there has been significant progress, the physical properties and potential fragmentation of accretion disks around high-mass protostars remain poorly constrained.…

astro-ph.GA2025

Filamentary accretion flows in high-mass star-forming clouds

J. -E. Schneider, H. Beuther, C. Gieser +11

We quantify the gas flows from a scale of up to several parsecs down to the sub-parsec scale along filamentary structures in the three high-mass star-forming regions G75.78, IRAS21…

astro-ph.GA2025★ 3 cited

From theory to observation: understanding filamentary flows in high-mass star-forming clusters

M. R. A. Wells, R. Pillsworth, H. Beuther +2

Here we use data from multi-scale galactic MHD simulations to observe filaments and star forming clumps on 10's of pc scales and investigate flow rate relationships along, and onto…

astro-ph.GA2021★ 22 cited

Fragmentation and kinematics in high-mass star formation: CORE-extension targeting two very young high-mass star-forming regions

H. Beuther, C. Gieser, S. Suri +24

Context: The formation of high-mass star-forming regions from their parental gas cloud and the subsequent fragmentation processes lie at the heart of star formation research. Aims:…

astro-ph.GA2021★ 28 cited

Multi-scale view of star formation in IRAS 21078+5211: From clump fragmentation to disk wind

L. Moscadelli, H. Beuther, A. Ahmadi +23

In the massive star-forming region IRAS 21078+5211, a highly fragmented cluster (0.1~pc in size) of molecular cores is observed, located at the density peak of an elongated (1~pc i…