Cold atomic gas identified by H I self-absorption - Cold atomic clouds toward giant molecular filaments

Open Access

Fig. 5

Histograms of fit line widths. The panels show for each of the six giant filament regions the normalized histogram of FWHM line widths of HISA and ¹³CO in black and blue, respectively. The black and blue vertical dashed lines mark the spectral resolution limit of the HISA and ¹³CO data, respectively.

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