Table 1
Fit parameters for the photoevaporative gas surface density profile.
| M★ (M⊙) | a | b | c | d | e | f | g |  |
LX (1029 erg s−1) |
|---|---|---|---|---|---|---|---|---|---|
| 1.0 | −0.6344 | 6.3587 | −26.1445 | 56.4477 | −67.7403 | 43.9212 | −13.2316 | 3.86446 | 20.42 |
| 0.5 | −1.2320 | 10.8505 | −38.6939 | 71.2489 | −71.4279 | 37.8707 | −9.3508 | 1.90460 | 7.02 |
| 0.3 | −1.3206 | 13.0475 | −53.6990 | 117.6027 | −144.3769 | 94.7854 | −26.7363 | 1.17156 | 3.20 |
| 0.1 | −3.8337 | 22.9100 | −55.1282 | 67.8919 | −45.0138 | 16.2977 | −3.5426 | 0.37588 | 0.59 |
Notes. Fit parameters taken from Picogna et al. (2021). The Ṁw values here are referred to as ‘nominal values’ and represent the Ṁw(M★, LX,soft) from Equation (6). Additionally shown are the X-ray luminosities for the different stellar masses, calculated with Equation (7).
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