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20232026
most citedDynamical Accretion Flows -- ALMAGAL: Flows along filamentary structures in high-mass star-forming clusters

30 citations · 67 across the 10 of their papers we have counts for

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6 papers · 1 filter

astro-ph.GA2025

CASCADE: Filamentary accretion flows in Cygnus X DR20

M. Sawczuck, H. Beuther, S. Suri +11

Aims. We investigate the role of filaments in high-mass star formation, whether gas flows from large to small scales along them, and what their properties might reveal about the re…

astro-ph.GA2025★ 5 cited

ALMAGAL V. Relations between the core populations and the parent clump physical properties

D. Elia, A. Coletta, S. Molinari +54

Context. The fragmentation of massive molecular clumps into smaller, potentially star-forming cores plays a key role in the processes of high-mass star formation. The ALMAGAL proje…

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.GA2025★ 9 cited

ALMAGAL IV. Morphological comparison of molecular and thermal dust emission using the histogram of oriented gradients (HOG) method

C. Mininni, S. Molinari, J. D. Soler +46

The study of molecular line emission is crucial to unveil the kinematics and the physical conditions of gas in star-forming regions. Our aim is to quantify the reliability of using…

astro-ph.GA2025

ALMAGAL III. Compact source catalog: Fragmentation statistics and physical evolution of the core population

A. Coletta, S. Molinari, E. Schisano +49

The mechanisms behind the fragmentation of high-mass dense clumps into compact star-forming cores are fundamental topics in current astrophysical research. The ALMAGAL survey provi…