Anisotropy in the carbon monoxide (CO) line emission across the Milky Way’s disk

Open Access

Fig. 5

Comparison of filament anisotropy in 10^° × 10^° regions from 7.^′5-resolution Dame et al. (2001) ¹²CO(1–0) observations (left), and in 2^° × 2^° regions from 49^′′-resolution ¹²CO(1–0) observations of the MWISP survey, for velocity channel widths of 1.5 km s⁻¹ (middle) and 0.16 km s⁻¹ (right), as reported by Soler et al. (2021).

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