Cosmological formation and chemical evolution of an elliptical galaxy

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Table 3:

Mass in stars formed in the last 1.0 and 6.2 Gyr for all the models compared with the total number of stars. Observed values by Kaviraj (2008b).
Model	M_* [ $M_{\odot}$ ] (last 1.0 Gyr [z = 0.08])	M_* [ $M_{\odot}$ ] (last 6.2 Gyr [z = 0.7])	M_* [ $M_{\odot}$ ] (13.12 Gyr)
1	4.17 $\times$ 10⁸ (0.21%)	3.66 $\times$ 10⁹ (1.85%)	1.98 $\times$ 10¹¹
2	0.00 (0.00%)	0.00 (0.00%)	1.58 $\times$ 10¹¹
3	7.95 $\times$ 10⁹ (4.25%)	5.54 $\times$ 10¹⁰ (29.63%)	1.87 $\times$ 10¹¹
Kaviraj (2008b)	1-6%	5-13%

Source LaTeX | All tables | In the text

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