Fig. 3
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Histograms of angular alignment deviations according to Eq. (5) for filamentary structures. Top left: Planck 857 GHz compared with Planck 353 GHz and angular orientations according Eq. (4), |b| > 20°. Top right: Planck 857 GHz compared with H I column densities for |vLSR| < 50 km s−1, |b| > 20°. Center left: Planck 857 GHz compared with best fit single channel H I filaments, all sky. Center right: Planck 857 GHz compared with best fit single channel H I filaments, |b| > 20°. Bottom left: Planck 857 GHz compared with best fit H I filaments at a channel width of 16 km s−1, all sky. Bottom right: Planck 857 GHz compared with best fit H I filaments at a channel width of 16 km s−1, |b| > 20°.
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