Table 8: Parameters for main sequence evolution for different progenitor masses $M_{\star }$ (from Chevalier 1999 and references therein). $\dot{M}_{{\rm loss}}$ is the mass loss rate, $L_{{\rm w}}$ is the mechanical wind luminosity, $t_{{\rm ms}}$ is the main-sequence age and  $r_{{\rm b}}$ is the maximum size of the wind bubble.
$M_{\star }$ Spectral $\dot{M}_{{\rm loss}}$ $L_{{\rm w}}$ $t_{{\rm ms}}$ $r_{{\rm b}}$
( ${M}_{\odot}$) type ( ${M}_{\odot} \: {\rm yr}^{-1}$) (erg s-1) (yr) (pc)
12 B1 V $6 \times 10^{-9}$ $9.3 \times 10^{32}$ $1.3 \times 10^{7}$ 5.3
16 B0 V $6 \times 10^{-8}$ $9.3 \times 10^{33}$ $0.9 \times 10^{7}$ 10.0


Source LaTeX | All tables | In the text