activity
20172026
most citedFragmentation and disk formation in high-mass star formation: The ALMA view of G351.77-0.54 at 0.06" resolution

44 citations · 64 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.EP2026★ 4 cited

The role of detailed gas and dust opacities in shaping the evolution of the inner disc edge subject to episodic accretion

Michael Cecil, Mario Flock, Mykola G. Malygin +4

We investigate the effects of different dust and gas opacity descriptions on the structure and evolution of the inner regions of protoplanetary discs. The influence on the episodic…

astro-ph.SR2026

The Structure and Kinematics of Three Class 0 Protostellar Jets from JWST

Samuel A. Federman, S. Thomas Megeath, Alessio Caratti o Garatti +20

We present observations of jets within 2000 au of three deeply embedded protostars using 2.9-27 micron observations with JWST. These observations show the morphologies and kinemati…

astro-ph.GA2025

Detection of a septuple stellar system in formation via disk fragmentation

Shanghuo Li, Henrik Beuther, André Oliva +15

Stellar multiple systems play a pivotal role in cluster dynamics and stellar evolution, leading to intense astronomical phenomena like X-ray binaries, gamma-ray bursts, Type Ia sup…

astro-ph.SR2024★ 16 cited

Mixing is easy: New insights for cosmochemical evolution from pre-stellar core collapse

Asmita Bhandare, Benoît Commerçon, Guillaume Laibe +5

Signposts of early planet formation are ubiquitous in substructured young discs. Dense, hot and high-pressure regions formed during gravitational collapse process, integral to star…

astro-ph.GA2024

Observations of high-order multiplicity in a high-mass stellar protocluster

Shanghuo Li, Patricio Sanhueza, Henrik Beuther +13

The dominant mechanism forming multiple stellar systems in the high-mass regime (M 8 ) remained unknown because direct imaging of multiple protostellar s…

astro-ph.GA2017★ 44 cited

Fragmentation and disk formation in high-mass star formation: The ALMA view of G351.77-0.54 at 0.06" resolution

H. Beuther, A. J. Walsh, K. G. Johnston +4

Aims: We resolve the small-scale structure around the high-mass hot core region G351.77-0.54 to investigate its disk and fragmentation properties. Methods: Using ALMA at 690GHz wit…