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Fig. B.2
Observations of the [CI] 1−0 and CO 3−2 transitions towards HD 100546 and four nearby reference positions (offset by ± 5′′ East/West and ± 10′′ North/South, as shown in Fig. B.1). The emission strongly peaks at the disk and the red and blue peaks show variation expected from a Keplerian disk observed at the various offsets.
This figure is made of several images, please see below:
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