Table 1
GB PNe model results and literature data for analysed nebulae.
| PN G | Name | log Tbb | Rout | Vaver | tkin | Mcspn |
|
O/H | Ref. | |||
| [K] | [pc] | [km s-1] | [kyr] | [M⊙] | [M⊙] | 12+logx | ||||||
|
|
||||||||||||
| 001.7-04.4 | H 1-55 | 4.53 | 0.07 | 26 | 1.88 | 0.603 | 0.565 | 8.45 | 1 | |||
| 002.3-03.4 | H 2-37 | 5.07 | 0.12 | 29 | 2.89 | 0.628 | 0.590 | 8.06 | 1 | |||
| 002.8+01.7 | H 2-20 | 4.50 | 0.065 | 29 | 1.57 | 0.607 | 0.569 | 9.26 | 2 | |||
| 002.9-03.9 | H 2-39 | 5.04 | 0.11 | 39 | 1.97 | 0.639 | 0.601 | 8.41 | 1 | |||
| 003.1+03.4 | H 2-17 | 4.49 | 0.08 | 24 | 2.33 | 0.592 | 0.555 | 7.44 | 2 | |||
| 003.6+03.1 | M 2-14 | 4.63 | 0.045 | 16 | 1.96 | 0.609 | 0.571 | 8.56 | 3 | |||
| 003.8+05.3 | H 2-15 | 4.89 | 0.12 | 17 | 4.93 | 0.596 | 0.558 | 8.66 | 2 | |||
| 004.1-03.8 | KFL 11 | 4.76 | 0.08 | 22 | 2.54 | 0.609 | 0.572 | 8.39 | 1 | |||
| 004.8+02.0 | H 2-25 | 4.49 | 0.10 | 18 | 3.88 | 0.575 | 0.537 | 8.33 | 3 | |||
| 006.1+08.3 | M 1-20 | 4.81 | 0.044 | 16 | 1.92 | 0.623 | 0.585 | 8.53 | 3 | |||
| 006.3+04.4 | H 2-18 | 4.71 | 0.11 | 46 | 1.67 | 0.620 | 0.583 | 8.56 | 1 | |||
| 006.4+02.0 | M 1-31 | 4.68 | 0.04 | 19 | 1.47 | 0.623 | 0.585 | 8.91 | 1 | |||
| 008.2+06.8 | He 2-260 | 4.44 | 0.02 | 12 | 1.16 | 0.613 | 0.575 | 8.00 | 3 | |||
| 008.6-02.6 | MaC 1-11 | 4.80 | 0.08 | 28 | 2.00 | 0.621 | 0.583 | – | ||||
| 351.1+04.8 | M 1-19 | 4.71 | 0.06 | 23 | 1.82 | 0.618 | 0.580 | 8.62 | 3 | |||
| 351.9-01.9 | Wray 16-286 | 4.92 | 0.06 | 13 | 3.22 | 0.613 | 0.575 | 8.74 | 3 | |||
| 352.6+03.0 | H 1-8 | 4.83 | 0.07 | 23 | 2.13 | 0.621 | 0.583 | 8.76 | 3 | |||
| 354.5+03.3 | Th 3-4 | 4.68 | 0.016 | 19 | 0.59 | 0.655 | 0.617 | 8.21 | 3 | |||
| 354.9+03.5 | Th 3-6 | 4.63 | 0.08 | 16 | 3.49 | 0.589 | 0.551 | – | ||||
| 355.9+03.6 | H 1-9 | 4.55 | 0.04 | 21 | 1.33 | 0.617 | 0.579 | 8.30 | 1 | |||
| 356.1-03.3 | H 2-26 | 5.18 | 0.11 | 20 | 3.84 | 0.627 | 0.588 | 8.34 | 2 | |||
| 356.5-03.6 | H 2-27 | 4.81 | 0.12 | 25 | 3.35 | 0.604 | 0.566 | – | ||||
| 356.8+03.3 | Th 3-12 | 4.51 | 0.03 | 9 | 2.33 | 0.594 | 0.556 | – | ||||
| 356.9+04.4 | M 3-38 | 5.09 | 0.02 | 9 | 1.55 | 0.651 | 0.613 | 8.39 | 1 | |||
| 357.1-04.7 | H 1-43 | 4.26 | 0.04 | 27 | 1.03 | 0.604 | 0.566 | 8.12 | 1 | |||
| 357.2+02.0 | H 2-13 | 4.95 | 0.09 | 8 | 7.86 | 0.585 | 0.547 | – | ||||
| 358.5-04.2 | H 1-46 | 4.75 | 0.04 | 14 | 2.00 | 0.618 | 0.579 | 8.27 | 1 | |||
| 358.5+02.9 | Al 2-F | 4.95 | 0.08 | 28 | 2.00 | 0.632 | 0.594 | – | ||||
| 358.7+05.2 | M 3-40 | 4.73 | 0.06 | 22 | 1.90 | 0.618 | 0.580 | – | ||||
| 358.9+03.4 | H 1-19 | 4.67 | 0.05 | 17 | 2.05 | 0.610 | 0.572 | 8.26 | 3 | |||
| 359.2+04.7 | Th 3-14 | 4.32 | 0.04 | 15 | 1.86 | 0.588 | 0.550 | – | ||||
Notes. The black-body temperature comes from photoionization modelling. The outer radius corresponds to the equatorial direction seen in the images observed with HST. The kinematical reconstruction provided the mass-averaged velocity and kinematical age. The methods for obtaining cspn masses in standard and accelerated cases are discussed in the text.
Reference. Abundance references: (1) Górny et al. (2009); (2) Stasińska et al. (1998); (3) Chiappini et al. (2009).
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