DUETS: Setting expectations for asteroseismic binaries and binary products with synthetic populations

Open Access

Table 4.

Counts of undermassive stars in the simulation adopting the MDS17 prescription, for evolutionary phases from MS to EAGB.

Phase	N	N_{lone pri}	N_sec	N $_{lone pri}^{\det}$ $_{\mathrm{lone~pri}}^{\mathrm{det}}$	N $_{\sec}^{\det}$ $_{\mathrm{sec}}^{\mathrm{det}}$	N $_{lone pri}^{\det}$ $_{\mathrm{lone~pri}}^{\mathrm{det}}$ /N^det	N $_{\sec}^{\det}$ $_{\mathrm{sec}}^{\mathrm{det}}$ /N^det	N^det
MS	3	0	3	0	0	0.00000	0.00000	7528
HG	5	0	5	0	1	0.00000	0.00031	3262
RGB	34	30	4	28	2	0.00132	0.00009	21 227
CHeB	290	287	3	279	1	0.01558	0.00006	17 906
EAGB	21	21	0	20	0	0.00850	0.00000	2354

Notes. Column names including the term “det” refer to the subsample of stars with detectable oscillations. The last column is for reference and is the same as in Table 2. There are no undermassive primary stars still in binaries, therefore the corresponding columns are not reported in the Table.

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