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

Open Access

Fig. 7

Brightness temperature maps of the dust continuum (left) and the ¹³CO .J=3−2 (middle panel) and ¹³CO .J=6−5 (right panel) transitions. The yellow stars in the centre indicate the approximate location of the host star, while the resolving beams are indicated by the white ellipses.

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