Extended Data Fig. 2: Comparison between the FAST observations and archival HI4PI data. | Nature Astronomy

Extended Data Fig. 2: Comparison between the FAST observations and archival HI4PI data.

From: A network of velocity-coherent filaments formed by supersonic turbulence in a very-high-velocity H i cloud

Extended Data Fig. 2

Upper panels: The integrated intensity maps of the HVC and foreground (fg) components of G165 by FAST and HI4PI. See Fig. 1 and Extended Data Fig. 1 for the integrated intensity maps of the VHVC component. Center panels: Channel maps of G165 VHVC by FAST with velocity resolution smoothed to 2 km/s (about one fiftieth of the velocity span). Lower panels: Channel maps of the foreground of G165 by FAST with velocity resolution smoothed to 0.3 km/s (about one fiftieth of the velocity span).

Source data

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