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Table 2

Summary of structure types and their statistical properties.

Structure Number Fraction Fraction Aspect Mean number Total number Mean number Total number Total number Fraction
type of structures of total flux ratio of pixels of CSC assoc. of CSC assoc. of MSF assoc. of MSF clumps of MSF clumps
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)

Clumps 370 0.28 0.06 2.09 44 325 0.9 11 12 0.02
Elongated 301 0.22 0.11 1.91 54 499 1.7 33 36 0.07
Filament 517 0.39 0.26 3.18 93 1495 2.9 43 63 0.12
Network 119 0.09 0.37 1.97 357 1609 13.5 29 80 0.15
Complex 32 0.02 0.21 1.81 444 574 17.9 9 32 0.06

Notes. The flux ratio is estimated by considering only the flux associated with structures where agreement is found. The fluxes are normalised with respect to the total flux in all the structures where agreement is found for the five main structure types. When determining the statistics for the association with the massive star forming(MSF) clumps we only consider structures outside of the inner 10° of the Galactic centre where the matching between ATLASGAL and massive star formation tracers is complete (for details see Urquhart et al. 2014c).

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