Table B.2.
Evolution of a zero-age post-CE binary towards the present-day properties of V1082 Sgr.
| Time | M1 | M2 | Type1 | Type2 | Orbital Period | Event |
|---|---|---|---|---|---|---|
| (Myr) | (M⊙) | (M⊙) | (d) | |||
| 0.0000 | 0.800 | 1.100 | WD | MS | 84.0000 | initial post-common-envelope binary |
| 5011.2289 | 0.800 | 1.098 | WD | SG | 84.1151 | secondary becomes a subgiant |
| 6492.0269 | 0.800 | 1.096 | WD | SG | 28.2261 | begin RLOF |
| 6516.0473 | 1.010 | 0.233 | WD | SG | 20.8487 | Binary looks like V1082 Sgr |
| 6864.6246 | 1.010 | 0.176 | WD | proto-WD | 19.0684 | end RLOF |
Notes. The quantities M1 and M2 and Type1 and Type2 are the masses and stellar types of the progenitors of the WD and its companion, respectively. Porb is the orbital period and the last column corresponds to the event occurring to the binary at the given time in the first column. The row in which the binary has the present-day properties of V1082 Sgr is highlighted in boldface. Abbreviations: MS (main-sequence star), SG (subgiant star), WD (white dwarf), RLOF (Roche lobe overflow).
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