Table 9
Observed and derived parameters of X-ray detected optical novae in M 31.
Optical measurements | X-ray measurements | Derived parameters | ||||||
|
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Namea | Brightnessb | t2Rc | SSS phase | LXd | k TBBe | Ejected mass | Burned mass | |
M31N | (mag Filter) | (d) | Turn on (d) | Turn off (d) | (1036 erg s-1) | (eV) | (10-5M⊙) | (10-6M⊙) |
|
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1995-09b | 15.6(Hα) | 1653 ± 81 | 3656 ± 273 | 16.1 ± 3.6 |
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6.1 ± 0.5 | ||
1995-11c | 16.3(Hα) | 762 ± 725 | 3609 ± 236 | 13.8 ± 3.3 |
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6.0 ± 0.4 | ||
1996-08b∗ | 16.1(Hα) | 1831 ± 49 | > 3829 | 5.6 ± 1.0 |
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> 6.4 | |
1997-11a∗ | 18.0(R) | 2027 ± 566 | > 3418 | 9.5 ± 1.4 |
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> 5.7 | ||
1999-10a | 17.5(W) | 357 ± 496 | 2203 ± 234 | 21.2 ± 1.6 |
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3.7 ± 0.4 | |
2000-07a | 16.8(R) | 22.4 | 162 ± 8 | 1904 ± 236 | 13.4 ± 0.7 | 6.7 ± 0.7 | 3.2 ± 0.4 | |
2001-01a∗ | 17.1(R) | < 1990 | > 2317 | 2.4 ± 0.5 | < 1016 | > 3.9 | ||
2001-10a∗ | 17.0(R) | 39.3 | 1089 ± 70 | > 1985 | 12.0 ± 2.0 |
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> 3.3 |
2003-11a | 16.9(R) | 22.0 | 327 ± 70 | 709 ± 235 | 27.6 ± 1.8 |
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1.2 ± 0.4 | |
2003-11b | 17.4(R) | 42.2 | 302 ± 70 | 684 ± 235 | 10.4 ± 1.3 |
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1.1 ± 0.4 | |
2004-05b∗ | 17.2(R) | 49.7 | 213 ± 11 | > 1028 | 45.8 ± 5.4 |
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11.7 ± 1.2 | > 1.72 |
2004-06c | 17.1(R) | 10.9 | 94 ± 70 | 476 ± 234 | 33.9 ± 2.0 |
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0.8 ± 0.4 | |
2004-11b+ | 16.6(R) | 32.0 | 68 ± 16 | 343 ± 235 | 16.2 ± 1.6 |
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0.6 ± 0.4 | |
2004-11g | 18.0(R) | 28.4 | 16 ± 16 | 343 ± 235 | 82.1 ± 3.0 |
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0.6 ± 0.4 | |
2004-11e | 17.6(R) | 34.6 | 44 ± 16 | 319 ± 235 | 35.9 ± 4.0 |
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0.5 ± 0.4 | |
2005-02a∗ | 17.7(W) | 236 ± 236 | > 751 | 56.4 ± 4.9 |
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> 1.25 | |
2006-04a∗ | 15.9(W) | 86 ± 19 | 132 ± 27 | 48.9 ± 2.0 |
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0.22 ± 0.05 | |
2006-06a∗+ | 17.6(R) | 106 ± 26 | 200 ± 25 | 10.3 ± 2.1 |
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0.33 ± 0.04 |
Notes.
∗ indicates novae with parameters mainly from this paper while the remaining objects are from PHS2007 (their Table 8) and we give updated turn-off times, ejected masses and burned masses, + indicates novae confirmed by optical spectra;
maximum observed magnitude (not necessarily peak magnitude), “W” indicates unfiltered magnitude;
time in days the nova R magnitude needs to drop 2 mag below peak magnitude (see Payne-Gaposchkin 1964);
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