The evolution of runaway stellar collision products

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Table 6:

Ejected mass and composition for the three computed merger sequences compared to the winds of a population of single stars corresponding to sequence 1.
	Single	Sequence 1				Sequence 2				Sequence 3
	Wind	Coll.	Wind	Remnant	Total	Coll.	Wind	Remnant	Total	Coll.	Wind	Remnant	Total
$\Delta M$	647.5	228.6	695.8	95.4	1020	191.8	549.9	83.5	825	142.3	456.6	102.0	701
H	0.4806	0.5648	0.4006	0.0899	0.4083	0.5599	0.3489	0.1944	0.3823	0.5521	0.3361	0.2025	0.3605
He	0.4965	0.4000	0.5794	0.8308	0.5627	0.4093	0.6311	0.7637	0.5930	0.4305	0.6439	0.7553	0.6168
C	0.0040	0.0012	0.0003	0.0306	0.0033	0.0090	0.0003	0.0133	0.0036	0.0004	0.0003	0.0184	0.0030
N	0.0092	0.0166	0.0132	0.0294	0.0155	0.0117	0.0133	0.0128	0.0129	0.0105	0.0134	0.0123	0.0127
O	0.0040	0.0013	0.0010	0.0060	0.0015	0.0044	0.0009	0.0081	0.0024	0.0013	0.0008	0.0050	0.0015

The first row lists the total mass $\Delta M$ (in solar units) lost through each of the three listed channels, the remaining rows give the abundances (by mass fraction) of H, He, C, N and O. For each sequence the first column lists the ejecta from the collision, the second column lists the integrated values for the stellar wind during the merger sequence, the third column lists the values for the evolution of the merger remnant after the merger sequence ended and the fourth column gives the combined yields from these channels.

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