APEX and NOEMA observations of H2S in nearby luminous galaxies and the ULIRG Mrk 231 - A possible relation between dense gas properties and molecular outflows

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Fig. 2.

NOEMA H₂S spectrum of Mrk 231 (zoomed in from Fig. 1). The x axis is in km s⁻¹ relative to the central velocity (12642 km s⁻¹). Redshifted and blueshifted line-wing emission is indicated with corresponding colours. Other identified lines are indicated in the figure (same as in Fig. 1).

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