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Table 3.

Binaries with detectable oscillations produced by the simulation with the MDS17 distribution of binary initial parameters.

Phaselate Phaseearly N None Nseismo Nseismo/N late det $ _{\mathrm{late}}^{\mathrm{det}} $ Nseismo/N early det $ _{\mathrm{early}}^{\mathrm{det}} $ Nseismo/∑ N late det $ _{\mathrm{late}}^{\mathrm{det}} $ Nseismo/∑Nseismo
MS MS 59 228 2070 30 0.00399 0.00399 0.00057 0.19868
HG MS 7620 1023 2 0.00061 0.00027 0.00004 0.01325
HG 521 9 5 0.00153 0.00153 0.00010 0.03311
RGB MS 8738 5589 1 0.00005 0.00013 0.00002 0.00662
RGB 257 133 20 0.00094 0.00094 0.00038 0.13245
CHeB RGB 145 69 29 0.00162 0.00137 0.00055 0.19205
CHeB 65 2 53 0.00296 0.00296 0.00101 0.35099
EAGB RGB 12 8 3 0.00127 0.00014 0.00006 0.01987
CHeB 6 2 4 0.00170 0.00022 0.00008 0.02649
EAGB 4 0 4 0.00170 0.00170 0.00008 0.02649

Notes. All binaries are considered unresolved. Columns “phaselate” and “phaseearly” indicate the evolutionary phase of the most (late) and least (early) evolved star in the system, respectively. “N” is the total number of systems with the given phases for the most and least evolved star at the end of the simulation. “None” indicates the number of systems where only one component has detectable oscillations and “Nseismo” represents the counts of asteroseismic binaries. “Nseismo/N late det $ _{\mathrm{late}}^{\mathrm{det}} $” and “Nseismo/N early det $ _{\mathrm{early}}^{\mathrm{det}} $” are the fraction of asteroseismic binaries with respect to all stars with detectable oscillations in the phase of the most and least evolved star, respectively, and “Nseismo/N late det $ _{\mathrm{late}}^{\mathrm{det}} $” is also plotted in Figure 2. Finally, “Nseismo/∑Ndet” represents the fraction of asteroseismic binaries to the total number of stars with detectable oscillations, regardless of their evolutionary stage, and “Nseismo/∑Nseismo” is the fraction of each kind of asteroseismic binary.

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