Table 4.
Luminosities of the central stars of PNe obtained using different methods: model-dependent luminosities determined from heating rates, luminisities derived from Zanstra temperatures and stellar magnitudes, from the integrated spectral energy distribution, and constrained from abolute Hβ flux and nebular modeling.
| log LMOD | log L*/L⊙ (H I) | log LSED/L⊙ | log LSED/L⊙ | log L*/L⊙ | log L*/L⊙ | |
|---|---|---|---|---|---|---|
| Ref. | [1] | [2] | [3] | [4] | [5] | [1] |
| Jacoby LMC 17 | 3.39 | |||||
| MGPN LMC 35 | 3.20 | |||||
| MGPN LMC 39 | 3.759 | 3.70 | 3.47 | 3.50 | ||
| SMP LMC 26 | 3.60 | 3.32 | ||||
| SMP LMC 31 | 3.791 | 4.01 | 3.90 | 3.64 | ||
| SMP LMC 55 | 3.650 | 3.69 | 4.21 | |||
| SMP LMC 67 | 2.86 | 3.33 | ||||
| MGPN SMC 8 | 3.867 | 4.33 | 3.49 | 3.42 | ||
| SMP SMC 1 | 3.784 | 3.77 | ||||
| SMP SMC 12 | 2.84 | |||||
| SMP SMC 16 | 3.20 | |||||
| SMP SMC 28 | 3.28 |
Notes. For SMP LMC 64 and SMP LMC 104A, no data were found in the literature. The data in bold are the central stars showing temperature evolution, modeled in Table 3.
References. [1] this paper, [2] Villaver et al. (2003, 2004), [3] van Aarle et al. (2011), [4] Kamath et al. (2014), [5] Dopita & Meatheringham (1991).
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