The evolution of runaway stellar collision products

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Table 5:

Times t and secondary masses m₂ for the sub merger sequence leading to the secondary of collision 22 in the merger sequence in Table 1.
N	t	$M_{1,N\mbox{-}{\rm body}}$	$M_{1,{\rm mix}}$	M₂	$M_{\rm merger}$
1	0.88048	66.6	63.6	65.2	113.4
2	1.08887	131.8	110.4	16.4	114.1
	3.10786	106.2	75.4

Source LaTeX | All tables | In the text

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