Compact planetary nebulae in the Galactic disk: Analysis of the central stars

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Table A.3

Derived central star properties.

PNG name	T_{H I}	T_{He II}	TR	log (L_∗/L_⊙)	BC
	(10³ K)	(10³ K)

PN G000.8−07.6	47.8 ± 3.10	60.2 ± 1.39	1.26	2.96 ± 0.27	−5.03 ± 0.16
PN G014.0−05.5	42.9 ± 2.55	83.1 ± 2.73	1.94	2.88 ± 0.28	−5.99 ± 0.23
PN G021.1−05.9	137.2 ± 15.19	130.0 ± 6.76	0.95	2.48 ± 0.30	−7.32 ± 0.36
PN G025.3−04.6	34.8 ± 1.80	52.2 ± 1.10	1.50	3.79 ± 0.27	−4.61 ± 0.14
PN G026.5−03.0	32.2 ± 1.55	...	...	2.62 ± 0.29	−3.17 ± 0.33
PN G042.9−06.9	41.7 ± 0.98	51.4 ± 0.61	1.23^a	3.69 ± 0.27	−4.57 ± 0.08
PN G044.1+ 05.8	23.2 ± 1.70	...	...	1.91 ± 0.33	−2.20 ± 0.50
PN G048.5+ 04.2	68.2 ± 11.05	119.9 ± 10.33	1.76	2.84 ± 0.35	−7.08 ± 0.59
PN G052.9−02.7	41.9 ± 5.00	60.2 ± 2.68	1.44	2.26 ± 0.29	−5.03 ± 0.30
PN G053.3+ 24.0	71.1 ± 0.61	100.3 ± 1.60	1.41	3.42 ± 0.26	−6.55 ± 0.11
PN G059.9+ 02.0	27.2 ± 2.30	...	...	2.03 ± 0.35	−2.67 ± 0.58
PN G068.7+ 01.9	44.6 ± 5.55	...	...	1.91 ± 0.43	−4.14 ± 0.85
PN G068.7+ 14.8	37.9 ± 0.23	59.2 ± 0.46	1.56	4.12 ± 0.26	−4.98 ± 0.05
PN G079.9+ 06.4	56.9 ± 8.35	>105.1^b	2.01	>2.04^b	<−6.37
PN G097.6−02.4	46.1 ± 2.90	76.7 ± 2.35	1.66	2.87 ± 0.27	−5.75 ± 0.21
PN G098.2+ 04.9	68.3 ± 11.89	109.4 ± 9.30	1.60	2.17 ± 0.36	−6.81 ± 0.58
PN G104.1+ 01.0	53.5 ± 7.50	...	...^a	1.33 ± 0.46	−4.68 ± 0.96
PN G107.4−02.6	52.2 ± 7.20	107.8 ± 8.45	2.07	2.40 ± 0.34	−6.76 ± 0.54
PN G184.0−02.1	40.3 ± 0.22	...	...^a	2.62 ± 0.26	−3.84 ± 0.04
PN G263.0−05.5	36.8 ± 0.22	67.2 ± 0.74	1.83^a	2.42 ± 0.26	−5.36 ± 0.07
PN G264.4−12.7	40.1 ± 0.26	...	...	3.54 ± 0.26	−3.83 ± 0.04
PN G275.3−04.7	83.3 ± 0.77	112.0 ± 1.95	1.34	2.97 ± 0.27	−6.88 ± 0.12
PN G278.6−06.7	127.1 ± 10.33	102.5 ± 3.44	0.81	3.01 ± 0.29	−6.61 ± 0.23
PN G285.4+ 01.5	85.7 ± 7.61	...	...^a	2.11 ± 0.36	−6.08 ± 0.61
PN G285.4+ 02.2	80.8 ± 14.15	134.4 ± 12.74	1.66	2.58 ± 0.37	−7.42 ± 0.65
PN G286.0−06.5	39.9 ± 0.22	...	...^a	3.06 ± 0.26	−3.81 ± 0.04
PN G289.8+ 07.7	67.3 ± 5.36	109.1 ± 4.59	1.62	3.12 ± 0.29	−6.80 ± 0.29
PN G294.9−04.3	41.8 ± 0.27	48.5 ± 0.37	1.16	3.53 ± 0.26	−4.39 ± 0.05
PN G295.3−09.3	31.6 ± 0.16	...	...^a	3.74 ± 0.26	−3.12 ± 0.03
PN G296.3−03.0	97.4 ± 3.71	113.3 ± 2.73	1.16^a	2.81 ± 0.27	−6.91 ± 0.16
PN G309.0+ 00.8	54.8 ± 3.85	...	...^a	1.91 ± 0.32	−4.75 ± 0.48
PN G309.5−02.9	69.3 ± 12.15	99.6 ± 7.65	1.44	2.34 ± 0.35	−6.53 ± 0.53
PN G324.8−01.1	63.4 ± 9.85	...	...^a	1.00 ± 0.50	−5.19 ± 1.06
PN G327.1−01.8	41.4 ± 2.40	...	...^a	2.52 ± 0.31	−3.92 ± 0.40
PN G327.8−06.1	30.2 ± 0.17	...	...	3.34 ± 0.26	−2.98 ± 0.04
PN G334.8−07.4	29.7 ± 0.11	...	...^a	3.25 ± 0.26	−2.93 ± 0.03
PN G336.9+ 08.3	26.6 ± 1.10	...	...	2.59 ± 0.28	−2.61 ± 0.28
PN G340.9−04.6	50.3 ± 6.93	...	...	2.30 ± 0.46	−4.50 ± 0.94
PN G341.5−09.1	29.0 ± 1.25	...	...	2.97 ± 0.29	−2.86 ± 0.30
PN G343.4+ 11.9	36.6 ± 1.95	72.6 ± 2.0	1.98	3.58 ± 0.27	−5.59 ± 0.19
PN G344.2+ 04.7	34.8 ± 0.21	...	...^a	3.27 ± 0.26	−3.40 ± 0.04
PN G344.8+ 03.4	33.0 ± 3.30	...	...	2.27 ± 0.38	−3.25 ± 0.68
PN G345.0+ 04.3	29.2 ± 0.13	...	...	3.06 ± 0.29	−2.88 ± 0.30
PN G348.4−04.1	38.3 ± 2.10	...	...^a	2.42 ± 0.30	−3.69 ± 0.38
PN G351.3+ 07.6	31.4 ± 1.45	...	...	3.47 ± 0.29	−3.10 ± 0.32
PN G356.5+ 01.5	38.0 ± 4.20	...	...	1.21 ± 0.40	−3.67 ± 0.76
PN G358.6+ 07.8	35.4 ± 1.85	...	...	2.68 ± 0.30	−3.46 ± 0.36

Notes.

^(a)

May be optically thick in H Lyman based on surface brightness.

^(b)

I(4686) > 90 suggests nebula is optically thin in He⁺, so T(He ii) and L(He ii) are lower limits.

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