A search for Galactic post-asymptotic giant branch stars in Gaia DR3

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Table A.3

Astrometric and evolutionary parameters for the 29 unconfirmed post-AGB candidates.

Num	Distance (pc)	Low Dist. (pc)	High Dist. (pc)	A_V	T(eff) (K)	Flag (T)	Lo𝑔[L]		Lo𝑔[L]_min	SED	Flag
6	4007	3509	4603	0.09	3500	T1	3.19	3.05	3.33	stellar	H
8	7877	7285	8653	< 0.01	7250	T2	2.92	2.83	3.01	stellar	H
16	7633	6920	8251	1.40	11000	T3(1)	3.12	3.03	3.20	stellar	H
23	2569	2382	2815	0.20	11750	T2	2.46	2.38	2.54	stellar	H
32	2138	2058	2229	0.70	9500	T3(2)	3.16	3.12	3.19	stellar	H
44	2568	2429	2706	0.30	7500	T3(3)	2.99	2.94	3.04	stellar	H
46	4893	4514	5338	0.60	6750	T3(4)	3.19	3.11	3.27	stellar	H
48	1446	1391	1510	0.85	22000	T3(5)	2.56	2.52	2.60	stellar	_-
57	945	921	964	0.40	6500	T3(6)	2.84	2.82	2.86	disc	_-
61	937	926	947	1.00	5750	T3(7)	2.06	2.05	2.07	shell	_-
66	1982	1915	2056	0.66	3750	T3(8)	2.37	2.33	2.40	shell	_-
69	1952	1895	2002	0.69	3750	T1	2.63	2.60	2.65	shell	_-
73	5266	4836	5721	4.00	1000	T3(8)	3.07	2.99	3.15	shell	-
80	3226	3025	3469	5.55	6000	T1	2.76	2.70	2.83	shell	-
81	2504	2408	2629	3.28	6750	T1	2.45	2.41	2.49	shell	-
83	1978	1856	2105	2.50	4000	T3(9)	3.01	2.95	3.06	disc	-
86	4277	3572	5089	5.80	8750	T3(8)	3.00	2.81	3.19	shell	-
87	5204	4054	6718	2.00	3500	T3(8)	1.96	1.64	2.27	shell	-
88	2533	2306	2812	4.53	3750	T1	2.94	2.84	3.04	shell	-
90	4882	4170	5705	3.00	4250	T3(8)	2.27	2.10	2.43	shell	-
91	5991	5520	6694	1.76	8250	T1	3.01	2.91	3.11	shell	-
100	4898	4294	5685	4.79	5750	T1	3.01	2.87	3.16	disc	-
101	6087	5536	6736	0.67	3500	T3(8)	3.15	3.06	3.25	shell	-
105	1694	1631	1768	5.34	4250	T1	2.50	2.46	2.53	disc	-
110	5710	4998	6635	< 0.01	14000	T3(10)	2.79	2.64	2.94	stellar	H
130	1365	1313	1420	0.90	4750	T2	3.21	3.16	3.27	shell	-
149	6299	5704	7065	0.47	4000	T3(9)	3.06	2.95	3.16	stellar	H
154	4714	4378	5080	0.38	4000	T1	3.29	3.22	3.36	stellar	-
155	2123	1943	2310	0.49	3500	T1	2.88	2.80	2.96	stellar	-

Notes. (H): Suspected Halo star.

References. Temperatures are: (T1) obtained from SED fitting with A_V from Stassun (2019), (T2): derived from Simbad spectral types, (T3): obtained from the literature (mainly for spectroscopic measurements): (1): Mooney et al. (2004), (2): Venn et al. (1998), (3): Kamath et al. (2022), (4): Gonzalez & Wallerstein (1992), (5): Hunger & Kaufmann (1973), (6): Kluska et al. (2022), (7): Ting et al. (2019), (8): Suárez et al. (2006), (9): Steinmetz et al. (2020), (10): Quin & Lamers (1992).

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