activity
20152025
most citedDisruption of the Orion Molecular Core 1 by the stellar wind of the massive star Ori C

140 citations · 1.3k across the 31 of their papers we have counts for

collaborators

31 papers

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.GA2023★ 25 cited

Kinematics and stability of high-mass protostellar disk candidates at sub-arcsecond resolution -- Insights from the IRAM NOEMA large program CORE

Aida Ahmadi, H. Beuther, F. Bosco +28

The fragmentation mode of high-mass molecular clumps and the accretion processes that form the most massive stars () are still not well understood. To this end,…

astro-ph.IM2023★ 28 cited

Data Combination: Interferometry and Single-dish Imaging in Radio Astronomy

Adele Plunkett, Alvaro Hacar, Lydia Moser-Fischer +11

Modern interferometers routinely provide radio-astronomical images down to subarcsecond resolution. However, interferometers filter out spatial scales larger than those sampled by…

astro-ph.GA2022★ 17 cited

ALMA Fragmented Source Catalogue in Orion (FraSCO) I. Outflow interaction within an embedded cluster in OMC-2/FIR3, FIR4, and FIR5

Asako Sato, Satoko Takahashi, Shun Ishii +6

We present a high angular resolution () and wide-field () image of the 1.3-mm continuum, CO( = 2--1) line, and SiO( = 5--4) line emissions toward an…

astro-ph.GA2022★ 17 cited

The Cygnus Allscale Survey of Chemistry and Dynamical Environments: CASCADE: Overview and first results toward DR20 from the Max Planck IRAM Observatory program (MIOP)

H. Beuther, F. Wyrowski, K. M. Menten +8

Context: While star formation on large molecular cloud scales and on small core and disk scales has been investigated intensely over the past decades, the connection of the large-s…

astro-ph.GA2022★ 28 cited

FEEDBACK from the NGC7538 HII region

H. Beuther, N. Schneider, R. Simon +10

Context: How do expanding HII regions interact with their environmental cloud? This is one of the central questions driving the SOFIA legacy program FEEDBACK. Here, we present a ca…