activity
20072026
most citedInterferometric multi-wavelength (sub)millimeter continuum study of the young high-mass protocluster IRAS05358+3543

79 citations · 182 across the 10 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2026

The Cygnus Allscale Survey of Chemistry and Dynamical Environments: CASCADE: VI. Molecular outflows in the DR21 ridge

I. M. Skretas, A. Karska, F. Wyrowski +8

Star formation takes place in varied environments, from isolated clumps to massive molecular cloud complexes. However, whether the environment in which a star forms has any effect…

astro-ph.GA2026★ 1 cited

Exploring the interplay between molecular and ionized gas in HII regions

S. Khan, A. M. Jacob, M. R. Rugel +8

We aim to constrain the kinetic temperature and H volume density of massive star-forming clumps associated with HII regions using multiple para-HCO transitions. In addition…

astro-ph.GA2025

A global view on star formation: The GLOSTAR Galactic plane survey XII. Effelsberg's continuum view and data release

Y. Gong, W. Reich, M. R. Rugel +24

Extended radio continuum emission and its linear polarization play a key role in probing large-scale structures of synchrotron and free-free emission in the Milky Way. Despite the…

astro-ph.GA2025

A multiscale evolutionary study of molecular gas in STARFORGE. I. Synthetic observations of SEDIGISM-like molecular clouds

K. R. Neralwar, D. Colombo, S. Offner +6

Molecular clouds are active sites of star formation in galaxies, and their formation and evolution are largely affected by stellar feedback. This includes outflows and winds from n…

astro-ph.GA2025★ 5 cited

UV-irradiated outflows from low-mass protostars in Ophiuchus with JWST/MIRI

I. M. Skretas, A. Karska, L. Francis +7

The main accretion phase of protostars is characterized by the ejection of material in the form of jets/outflows. External UV irradiation can potentially have a significant impact…

astro-ph.GA2025

High-resolution APEX/LAsMA CO and CO (3-2) observation of the G333 giant molecular cloud complex : III. Decomposition of molecular clouds into multi-scale hub-filament structures

J. W. Zhou, J. S. Urquhart, F. Wyrowski +3

We decomposed the G333 complex and the G331 giant molecular cloud into multi-scale hub-filament systems (HFs) using the high-resolution CO (32) data from LAsMA observatio…

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.GA2017★ 53 cited

The ATLASGAL survey: The sample of young massive cluster progenitors

T. Csengeri, S. Bontemps, F. Wyrowski +5

The progenitors of high-mass stars and clusters are still challenging to recognise. Only unbiased surveys, sensitive to compact regions of high dust column density, can unambiguous…

astro-ph.GA2015

The first Galaxy scale hunt for the youngest high-mass protostars

T. Csengeri, S. Bontemps, F. Wyrowski +17

The origin of massive stars is a fundamental open issue in modern astrophysics. Pre-ALMA interferometric studies reveal precursors to early B to late O type stars with collapsing e…

astro-ph.GA2009★ 22 cited

Evidence of triggered star formation in G327.3-0.6. Dust-continuum mapping of an infrared dark cloud with P-ArTéMiS

V. Minier, Ph. André, P. Bergman +17

Aims. Expanding HII regions and propagating shocks are common in the environment of young high-mass star-forming complexes. They can compress a pre-existing molecular cloud and tri…

astro-ph2007★ 79 cited

Interferometric multi-wavelength (sub)millimeter continuum study of the young high-mass protocluster IRAS05358+3543

H. Beuther, S. Leurini, P. Schilke +3

The young massive star-forming region IRAS05358+3543 was observed at high-spatial resolution in the continuum emission at 3.1 and 1.2mm with the Plateau de Bure Interferometer, and…