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Table 1.
Parameters of the systems modelled.
| Scenario |
||||||
|---|---|---|---|---|---|---|
| Parameter | Symbol | B0–0.5–d | B1–1–h | B1–1–d | B1–1–mc | B2–60–d |
| Peculiar velocity | V⋆ [km s−1] | 500 | 1000 | 1000 | 1000 | 60 000 |
| Ambient density | nISM [cm−3] | 10 | 0.1 | 10 | 100 | 10 |
| Ambient mean molecular weight | μISM | 1.28 | 1.28 | 1.28 | 2.35 | 1.28 |
| Ambient temperature | TISM [K] | 100 | 100 | 100 | 10 | 100 |
| Spectral type | B0 | B1 | B1 | B1 | B2 | |
| Wind velocity | vw [km s−1] | 1500 | 1200 | 1200 | 1200 | 1000 |
| Wind mass-loss rate | Ṁw [M⊙ yr−1] | 10−8 | 10−9 | 10−9 | 10−9 | 10−10 |
| Stellar radius | R⋆ [R⊙] | 5.5 | 4.8 | 4.8 | 4.8 | 4 |
| Stellar temperature | T⋆ [kK] | 29 | 25 | 25 | 25 | 20 |
| Distance to BS apex | R0 [AU] | 792 | 1120 | 112 | 26.2 | 0.54 |
Notes. The values of vw and Ṁw are taken from Krtička (2014) and Kobulnicky et al. (2019), and R⋆ and T⋆ from Harmanec (1988). We assume solar abundances.
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