Panel a: spatial distribution of the 26 ALMA compact cores (magenta, pink, orange, yellow, green, red, green, and light blue circles) and 7 ArTéMiS clumps (larger black dashed ellipses – see Sect. 4.1) embedded in the NGC 6334 main filament, overlaid on the ALMA 3.1 mm continuum image (grayscale and same solid contours as in Fig. 1). The black dashed contour shows an ArTéMiS 350 μm continuum emission level of 5 Jy/8′′-beam. The green curve marks the crest of the dusty filament traced with DisPerSE in the ArTéMiS 350 μm continuum map (André et al. 2016, see Fig. 1c). The red curves mark the area within ±30′′ (or ±0.25 pc) from this filament crest. Panel b: spatial distribution of the N2H+(1–0) velocity-coherent fiber-like sub-structures F-1 (blue, integrated over the velocity range −3 to −2.4 km s−1) and F-2 (red, integrated over the velocity range −2.0 to −1.2 km s−1) in the NGC 6334 filament. In panel a, the seven groups of ALMA 3.1 mm compact sources found by the nearest neighbor separation algorithm (see Sect. 4.1 and Fig. 8) are indicated by small circles of different colors. The green curve is the same as in panel a.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.