A CO funnel in the Galactic centre: Molecular counterpart of the northern Galactic chimney

Open Access

Fig. A.3.

Spectra of CS and ¹³CS J = 2 − 1 emission towards four positions along the GCMF restricted to a velocity range of −30 to 30 km s⁻¹ for better visualisation of the emission features. ¹³CS spectra are scaled by a factor of 6. The blue dashed line corresponds to the peak of the ¹³CS line.

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