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

Open Access

Fig. 5

M–L distribution of the nearby HGBS filaments (triangles; Arzoumanian et al. 2019, ; priv. commun.) and fibers (circles Hacar et al. 2023; Socci et al. 2024a,b) color-coded by their mean column density Σ (left panel) and aspect ratio A (right panel). Labels and lines are similar to those in Fig. 4.

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