Table 1
Values for and
as a function of Z.
Z | ![]() |
![]() |
||||
---|---|---|---|---|---|---|
BPASS(a) | Gen,rot(b) | LC18,rot(c) | LC18,non-rot(d) | D03(e) | ||
0.014 | 18 | 28 | 23 | 18(f) | 23 | 33 |
0.006 | 24 | 33 | 75 | 28 | 75 | 43 |
0.002 | 37 | 55 | 105 | 35 | 100 | 48 |
Notes. (a) Non-rotating BPASS V2.0 single-star tracks Eldridge et al. (2008); Eldridge & Stanway (2016), (b) rotating (vrot, i = 40% critical) Geneva tracks, Georgy et al. (2015), (c)rotating (vrot, i = 150 km s−1) FRANEC tracks, Limongi & Chieffi (2018). Values for Z = 0.006 are obtained through linear interpolation between Z = 0.002, 0.014, (d) non-rotating FRANEC tracks Limongi & Chieffi (2018), (e)non-rotating STARS tracks, Dray & Tout (2003), (f)these tracks imply self-stripping already at initial masses of ≈15 M⊙. However, following our strict definition, cannot be smaller than
, and hence we set
=
.
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