Characterising the molecular line emission in the asymmetric Oph-IRS 48 dust trap: Temperatures, timescales, and sub-thermal excitation

Open Access

Fig. 9

Cartoon visualising our proposed radial vertical emission scheme, containing SO₂ (blue), ¹³CO (orange), and H₂CO and CH₃OH (red). The radial and vertical emission locations are based on the derived temperatures, the proposed sliver theory, and the assumption that the ¹³CO emission is spatially resolved.

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