13 citations · 43 across the 6 of their papers we have counts for
7 papers
Emergence of high-mass stars in complex fiber networks (EMERGE) VII. Multi-Tracer Column Density Synthesis
Alvaro Hacar, Andrea Socci, Mario Tafalla +1
Obtaining accurate estimates of the gas column density is crucial to determine the physical conditions of the molecular gas in the Interstellar Medium. This paper…
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…
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…
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…
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…
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…
Another X-ray UFO without a momentum-boosted molecular outflow. ALMA CO(1-0) observations of the galaxy pair IRAS 05054+1718
F. Bonanomi, C. Cicone, P. Severgnini +8
We present ALMA CO(1-0) observations of the nearby LIRG galaxy pair IRAS05054+1718 with a new analysis of X-ray data collected between 2012 and 2021 using NuSTAR, Swift, and XMM-Ne…