Large-field CO (1–0) observations towards the Galactic historical supernova remnants: Shocked molecular clouds towards the Crab Nebula

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Fig. 6

HI4PI HI intensity image, integrated in the velocity range [5, 11] km s⁻¹. The contours start at 320 K km s⁻¹ and then increase in steps of 20 K km s⁻¹. The red contours show the CO emission in the velocity range [5, 11] km s⁻¹ (from Fig 3b), while the dashed yellow circle (radius of $0_{\cdot}^{\circ} 45$ $\[0^{\circ}_\cdot45\]$ ) shows the putative outer shocks from SN 1054 at a velocity of 15,000 km s⁻¹.

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