Table 1
Initial binary parameters M1, M2 and a for typical post-nova merger progenitors with for Z = 0.008, αCE = 0.2.
| M1/M⊙ | M2/M⊙ | a/R⊙ | Case | C/O |
|
MJ/M⊙ | M Bol,J |
|
|
|||||||
| 1.63 | 1.20 | 363.1 | COAL−A | 1.03 | 2.46 | 1.21 | −3.48 |
| 2.15 | 0.78 | 631.0 | COAL−B | 0.6 | 9.00 | 1.29 | −4.69 |
| 1.71 | 0.94 | 631.0 | CE−A | 1.17 | 2.09 | 1.02 | −2.25 |
| 2.05 | 1.39 | 524.8 | CE−B | 0.82 | 3.16 | 1.63 | −5.24 |
Notes. The post-nova merger emerges with surface C/O as given in Col. 5.
The J-suffix denotes the instant at which the merger has both C/O > 1 and
(J-star criteria) – thus
MJ and MBol,J respectively
denote the mass and bolometric magnitudes (Eq. (13)) of the post-nova merger when it classifies as a J-star.
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