most citedEmergence of high-mass stars in complex fiber networks (EMERGE) V. From filaments to spheroids: the origin of the hub-filament systems

8 citations · 9 across the 2 of their papers we have counts for

collaborators

5 papers

astro-ph.GA20248 cited

Emergence of high-mass stars in complex fiber networks (EMERGE) V. From filaments to spheroids: the origin of the hub-filament systems

A. Hacar, R. Konietzka, D. Seifried +7

Identified as parsec-size, gas clumps at the junction of multiple filaments, hub-filament systems (HFS) play a crucial role during the formation of young clusters and high-mass sta…

astro-ph.GA2024

Emergence of high-mass stars in complex fiber networks (EMERGE) IV. Environmental dependence of the fiber widths

A. Socci, A. Hacar, F. Bonanomi +2

Despite their variety of scales throughout the interstellar medium, filaments in nearby low-mass clouds show a characteristic width of 0.1 pc from the analysis of {\it Hersc…

astro-ph.IM20241 cited

New methods for ALMA angular-scale based observation scheduling, quality assessment, and beam shaping II: refinements

Dirk Petry, María Díaz Trigo, Rüdiger Kneissl +5

The Atacama Large Millimeter/submillimeter Array remains the largest mm radio interferometer observatory world-wide. It is now conducting its 11th observing cycle. In our previous…

astro-ph.GA2024

Emergence of high-mass stars in complex fiber networks (EMERGE) II. The need for data combination in ALMA observations

F. Bonanomi, A. Hacar, A. Socci +2

ALMA's high-resolution images allow to resolve the filamentary structure of the ISM down to few thousand au at kpc distances. We aim to systematically quantify the impact of the in…

astro-ph.GA2024

Emergence of high-mass stars in complex fiber networks (EMERGE). I. Early ALMA Survey: observations and massive data reduction

A. Hacar, A. Socci, F. Bonanomi +10

(Abridged) Recent molecular surveys have revealed a rich gas organization of sonic-like fibers in all kind of environments prior to the formation of low- and high-mass stars. This…