Table C.3
Radio observables obtained from RACS-low images for new and known bow shock candidates.
| id | Runaway Star | RMS | Image RMS | BMAJ | BMIN | RACS field |
|---|---|---|---|---|---|---|
| (µJy) | (µJy) | (″) | (″) | |||
| BS-GR9 | HD 41997 | 422 | 272 | 20.0 | 13.6 | 0606+18A |
| BS-GR35 | HD 64568 | 461 | 268 | 21.6 | 15.6 | 0741−25A |
| BS-GR71 | HD 89137 | 252 | 176 | 14.6 | 13.4 | 1027−50A |
| BS-GR75 | HDE 338 916 | 413 | 261 | 22.7 | 13.0 | 1955+25A |
| BS-GR93 | HD 116282 | 286 | 317 | 20.1 | 13.0 | 1314−62A |
| BS-GR40 | HD 46573 | 737 | 307 | 23.7 | 16.5 | 0624+00A |
| BS-GR70 | CPD −26 2716 | 424 | 268 | 21.6 | 15.6 | 0741−25A |
| BS-GR83 | HD 155775 | 911 | 376 | 13.6 | 12.8 | 1721−37A |
Notes. The RMS is measured in a 2′ circle centered at the position of the bow shock. Image RMS is median image RMS over the tile. BMAJ and BMIN are the beam’s major and minor axis size for each image, respectively. We only included here the radio non-detected bow shock candidates that contain all the stellar parameters and estimated nISM needed. We did not include here BS-GR51 because it has a clear radio detection, neither BS-GR72 because it is not visible by ASKAP. We included BS-GR83 because it does not have a clear radio detection. The horizontal line separates the new bow shock (top) from the known bow shock candidates (bottom).
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