Table 7.
Overview of UD measurements in the literature.
| Star | Distance | Distance | Variability | Period | Period | UD diam. | Flux | at freq. | UD |
|---|---|---|---|---|---|---|---|---|---|
| [pc] | Ref. | type | [days] | Ref. | [mas] | [mJy] | [GHz] | Ref. | |
| R Dor | 55 ± 3 | 1 | SRb | 332, 175 | 5 | 61.8 | 221.4 | 225 | 1 |
| W Hya |
![]() |
2 | Mira | 402 | VSX | 50 a | 210 a | 240 | 3 |
| Mira A | 100 ± 20 | 3 | Mira | 331 | VSX | 43.3 | 99.61 | 229.13 | 3 |
| R Leo | 100 ± 5 | 2 | Mira | 312 | VSX | 41.88 | 107.83 | 232.53 | 3 |
| R Lep |
![]() |
2 | Mira | 437 | VSX | 14.2 | 37.3 | 405.0 | 6 |
| CW Leo | 123 ± 14 | 4 | Mira | 630 | VSX | 53 b | 372 | 258 c | 7 |
Notes. (a) Values interpolated from higher and lower frequency observations. (b) Parameters given are for a Gaussian fit performed on the data, and hence are not directly comparable to UD fits. (c) Approximate estimates. 1: Vlemmings et al. (2024); 2: Andriantsaralaza et al. (2022); 3: Vlemmings et al. (2019); 4: Groenewegen et al. (2012); 5: Bedding et al. (1998); 6: Asaki et al. (2023); 7: Velilla-Prieto et al. (2023); VSX indicates a period taken directly from the VSX database.
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