#Table 1 - Reference values at t = 15Gyr for a 10^11 M_sun #theoretical CSP with changing star-formation properties^(a) #_________________________________________________________________ # beta b M*/L_CSP L_CSP^(b) Eo/Mo F^(c) # [M_sun/L_sun] [L_sun] x10^17 [erg/g] #_________________________________________________________________ 0.8 0.2 2.42 0.41 8.77 0.126 0.6 0.4 1.82 0.55 8.03 0.115 0.4 0.6 1.44 0.69 7.65 0.110 0.2 0.8 1.19 0.84 7.50 0.108 0.0 1.0 1.02 0.98 7.33 0.105 -0.2 1.2 0.89 1.12 7.21 0.103 -0.4 1.4 0.80 1.25 7.06 0.101 -0.6 1.6 0.72 1.38 6.94 0.099 -0.8 1.8 0.66 1.51 6.84 0.098 -1.0 2.0 0.61 1.64 6.77 0.097 #_________________________________________________________________ ^(a) Assuming SFR \propto t^-beta, and a birthrate b = 1-beta ^(b) For a 1 M_sun CSP ^(c) Burning efficiency factor F = (Eo/Mo)/K