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Table 3.
Overview of the morphological classification of the continuum images.
| Star | Classification | Notes | Sect. | Fig. |
|---|---|---|---|---|
| GY Aql | Unique | Bar to the south-east | 3.5.1 | 1 |
| R Aql | Extended, unique | Some extended emission around the star | 3.2 | 2 |
| IRC−10529 | Elongated, extended | Rectangular or bipolar extensions | 3.4 | 3 |
| W Aql | Extended, unique | Continuum flux seen near companion | 3.5.3 | 4 |
| SV Aqr | Unique | Asymmetric dust feature | 3.5.4 | 5 |
| U Del | Resolution-limited | Minimal signal in UD-subtracted map | 3.2 | 6 |
| π1 Gru | Unique | Companion seen in extended, tail of dust in its wake | 3.5.5 | 7 |
| U Her | Extended | Irregular extended distribution | 3.3.1 | 8 |
| R Hya | Extended | Strong detection | 3.3.2 | 9 |
| T Mic | Elongated? | Mostly round and compact | 3.4 | 10 |
| S Pav | Extended | Strong detection | 3.3.3 | 11 |
| IRC+10011 | Extended | Likely significant resolved-out flux | 3.3.4 | 12 |
| V PsA | Resolution-limited | 3.2 | 13 | |
| RW Sco | Resolution-limited | 3.2 | 14 | |
| KW Sgr | Resolution-limited/unique | Tentative detection of narrow extended dust feature | 3.2 | 15 |
| VX Sgr | Elongated? | More flux to the south than north | 3.4 | 16 |
| AH Sco | Unique | Possible dust shell or artefacts from resolved-out flux | 3.5.6 | 17 |
Notes. The ‘Sect.’ column gives the subsection in which each star is discussed in more detail.
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