Table 1. Open in new tab Basic data of...

								E(B − V)
(1) IRAS 02143+5852	133.8	−1.93	F7Ie	13.8	13.51	1.22	0.48	0.74	1.05		...	6000	−0.07	1,2,3
(2) IRAS 05089+0459	196.3	−19.5	M3I	14.08	13.13	1.74			0.14		...	3200	−2.24	1,4
(3) IRAS 05208−2035	222.8	−28.3		9.48	8.98	1.04	0.7:	0.3:	0.06	0.08	0.3 ± 0.2	4900	−0.33	5,6,7
(4) HD 46703	162.0	+19.	F7I	9.04	8.84	0.48	0.02	0.46	0.08	0.10	0.46 ± 0.20	6000	−0.06	1,7,8,9
(IRAS 06338+5333)
(5) HD 56126	206.7	+10.0	F5Ia	8.32	8.06	0.88	0.32	0.56	0.08	0.00	0.56 ± 0.20	6500	−0.03	1,10,11,12
(IRAS 07134+1005)
(6) IRAS 07140−2321	236.6	−5.4	F5I	10.73	10.49	0.43	0.23	0.20	0.59	0.57	0.57 ± 0.20	7000	0.0	1,13
(7) IRAS 07227−1320	228.7	+1.2	M1I	12.55	11.6	1.96	1.69	0.27	0.51	0.43	0.43 ± 0.20	3500	−1.45	1,14
(8) IRAS 08187−1905	240.6	+9.8	F6Ib/II	9.02	8.83	0.61	0.40	0.21	0.11	0.15	0.21 ± 0.05	6150	− 0.06	1,12,15
(9) HD 116745	309.1	+15.2	A7/A9e	10.79	10.68	0.29	0.13	0.16	0.13		0.16 ± 0.05	6950	−0.0	1,16
(10) IRAS 14325−6428	313.9	+4.1	F5I	12.0	11.27	0.56	0.32	0.24	0.64	0.89	0.89 ± 0.20	6400	−0.03	1,11,12
(11) IRAS 15210-6554	317.7	−7.7	K2I	11.85	11.72	(0.03)*	1.36		0.20		...	4310	−0.61	1
(12) HD 137569	21.9	+51.9	B9Iab:p	7.91	7.89	−0.05	...	0.0	0.05	0.01	0.01 ± 0.05	10500	−0.53	1,17,18
(13) BD +33 2642	52.7	+50.8	O7p	10.73	10.78	−0.12	−0.27	0.15	0.02	0.06	0.15 ± 0.05	20000	−1.66	1,19,20
(14) BD +32 2754	53.6	+41.5	F8	9.55	9.46	0.57	0.56	0.01	0.02	0.02	0.01 ± 0.05	5750	−0.09	1,14
(15) HD161796	77.1	+30.9	F3Ib	7.21	7.08	0.47	0.26	0.21	0.03	0.04	0.21 ± 0.05	6500	−0.03	1,9,12,21
(IRAS 17436+5003)
(16) BD −12 4970	018.0	+1.6	B0.5Ia	8.78	8.30	1.02	−0.21	1.23	2.71	1.58	1.23 ± 0.20	27000	−2.40	1
(17) IRAS 18075−0924	019.8	+4.7	—	13.9	12.47	1.4			1.41		...			1
(18) HD 178443	354.2	−21.5	F8	10.02	9.80	0.673	0.56	0.11	0.09		0.11 ± 0.05	5180	−0.09	1,22
(19) PHL 1580	031.3	−43.5	B0I	12.33	12.19	(0.14)*	−0.22		0.04	0.03	0.03 ± 0.05	24000	−2.8	1,23
(20) LS III +52 5	095.1	+0.8	OB-	(12.2)*	11.74	(0.46)*	−0.22		2.91	0.03	0.03 ± 0.05	25000	−2.9	1,24

E(B − V)

Star

l (°)

b (°)

Sp.

(B − V)

(B − V)₀ Sp

SFD

Adopted

T_eff (K)

B.C

Ref.^‡

(1) IRAS 02143+5852

133.8

−1.93

F7Ie

13.8

13.51

1.22

0.48

0.74

1.05

...

6000

−0.07

1,2,3

(2) IRAS 05089+0459

196.3

−19.5

M3I

14.08

13.13

1.74

0.14

...

3200

−2.24

1,4

(3) IRAS 05208−2035

222.8

−28.3

9.48

8.98

1.04

0.7:

0.3:

0.06

0.08

0.3 ± 0.2

4900

−0.33

5,6,7

(4) HD 46703

162.0

+19.

F7I

9.04

8.84

0.48

0.02

0.46

0.08

0.10

0.46 ± 0.20

6000

−0.06

1,7,8,9

(IRAS 06338+5333)

(5) HD 56126

206.7

+10.0

F5Ia

8.32

8.06

0.88

0.32

0.56

0.08

0.00

0.56 ± 0.20

6500

−0.03

1,10,11,12

(IRAS 07134+1005)

(6) IRAS 07140−2321

236.6

−5.4

F5I

10.73

10.49

0.43

0.23

0.20

0.59

0.57

0.57 ± 0.20

7000

0.0

1,13

(7) IRAS 07227−1320

228.7

+1.2

M1I

12.55

11.6

1.96

1.69

0.27

0.51

0.43

0.43 ± 0.20

3500

−1.45

1,14

(8) IRAS 08187−1905

240.6

+9.8

F6Ib/II

9.02

8.83

0.61

0.40

0.21

0.11

0.15

0.21 ± 0.05

6150

− 0.06

1,12,15

(9) HD 116745

309.1

+15.2

A7/A9e

10.79

10.68

0.29

0.13

0.16

0.13

0.16 ± 0.05

6950

−0.0

1,16

(10) IRAS 14325−6428

313.9

+4.1

F5I

12.0

11.27

0.56

0.32

0.24

0.64

0.89

0.89 ± 0.20

6400

−0.03

1,11,12

(11) IRAS 15210-6554

317.7

−7.7

K2I

11.85

11.72

(0.03)*

1.36

0.20

...

4310

−0.61

(12) HD 137569

21.9

+51.9

B9Iab:p

7.91

7.89

−0.05

...

0.0

0.05

0.01

0.01 ± 0.05

10500

−0.53

1,17,18

(13) BD +33 2642

52.7

+50.8

O7p

10.73

10.78

−0.12

−0.27

0.15

0.02

0.06

0.15 ± 0.05

20000

−1.66

1,19,20

(14) BD +32 2754

53.6

+41.5

9.55

9.46

0.57

0.56

0.01

0.02

0.01 ± 0.05

5750

−0.09

1,14

(15) HD161796

77.1

+30.9

F3Ib

7.21

7.08

0.47

0.26

0.21

0.03

0.04

0.21 ± 0.05

6500

−0.03

1,9,12,21

(IRAS 17436+5003)

(16) BD −12 4970

018.0

+1.6

B0.5Ia

8.78

8.30

1.02

−0.21

1.23

2.71

1.58

1.23 ± 0.20

27000

−2.40

(17) IRAS 18075−0924

019.8

+4.7

—

13.9

12.47

1.4

1.41

...

(18) HD 178443

354.2

−21.5

10.02

9.80

0.673

0.56

0.11

0.09

0.11 ± 0.05

5180

−0.09

1,22

(19) PHL 1580

031.3

−43.5

B0I

12.33

12.19

(0.14)*

−0.22

0.04

0.03

0.03 ± 0.05

24000

−2.8

1,23

(20) LS III +52 5

095.1

+0.8

OB-

(12.2)*

11.74

(0.46)*

−0.22

2.91

0.03

0.03 ± 0.05

25000

−2.9

1,24

								E(B − V)
(1) IRAS 02143+5852	133.8	−1.93	F7Ie	13.8	13.51	1.22	0.48	0.74	1.05		...	6000	−0.07	1,2,3
(2) IRAS 05089+0459	196.3	−19.5	M3I	14.08	13.13	1.74			0.14		...	3200	−2.24	1,4
(3) IRAS 05208−2035	222.8	−28.3		9.48	8.98	1.04	0.7:	0.3:	0.06	0.08	0.3 ± 0.2	4900	−0.33	5,6,7
(4) HD 46703	162.0	+19.	F7I	9.04	8.84	0.48	0.02	0.46	0.08	0.10	0.46 ± 0.20	6000	−0.06	1,7,8,9
(IRAS 06338+5333)
(5) HD 56126	206.7	+10.0	F5Ia	8.32	8.06	0.88	0.32	0.56	0.08	0.00	0.56 ± 0.20	6500	−0.03	1,10,11,12
(IRAS 07134+1005)
(6) IRAS 07140−2321	236.6	−5.4	F5I	10.73	10.49	0.43	0.23	0.20	0.59	0.57	0.57 ± 0.20	7000	0.0	1,13
(7) IRAS 07227−1320	228.7	+1.2	M1I	12.55	11.6	1.96	1.69	0.27	0.51	0.43	0.43 ± 0.20	3500	−1.45	1,14
(8) IRAS 08187−1905	240.6	+9.8	F6Ib/II	9.02	8.83	0.61	0.40	0.21	0.11	0.15	0.21 ± 0.05	6150	− 0.06	1,12,15
(9) HD 116745	309.1	+15.2	A7/A9e	10.79	10.68	0.29	0.13	0.16	0.13		0.16 ± 0.05	6950	−0.0	1,16
(10) IRAS 14325−6428	313.9	+4.1	F5I	12.0	11.27	0.56	0.32	0.24	0.64	0.89	0.89 ± 0.20	6400	−0.03	1,11,12
(11) IRAS 15210-6554	317.7	−7.7	K2I	11.85	11.72	(0.03)*	1.36		0.20		...	4310	−0.61	1
(12) HD 137569	21.9	+51.9	B9Iab:p	7.91	7.89	−0.05	...	0.0	0.05	0.01	0.01 ± 0.05	10500	−0.53	1,17,18
(13) BD +33 2642	52.7	+50.8	O7p	10.73	10.78	−0.12	−0.27	0.15	0.02	0.06	0.15 ± 0.05	20000	−1.66	1,19,20
(14) BD +32 2754	53.6	+41.5	F8	9.55	9.46	0.57	0.56	0.01	0.02	0.02	0.01 ± 0.05	5750	−0.09	1,14
(15) HD161796	77.1	+30.9	F3Ib	7.21	7.08	0.47	0.26	0.21	0.03	0.04	0.21 ± 0.05	6500	−0.03	1,9,12,21
(IRAS 17436+5003)
(16) BD −12 4970	018.0	+1.6	B0.5Ia	8.78	8.30	1.02	−0.21	1.23	2.71	1.58	1.23 ± 0.20	27000	−2.40	1
(17) IRAS 18075−0924	019.8	+4.7	—	13.9	12.47	1.4			1.41		...			1
(18) HD 178443	354.2	−21.5	F8	10.02	9.80	0.673	0.56	0.11	0.09		0.11 ± 0.05	5180	−0.09	1,22
(19) PHL 1580	031.3	−43.5	B0I	12.33	12.19	(0.14)*	−0.22		0.04	0.03	0.03 ± 0.05	24000	−2.8	1,23
(20) LS III +52 5	095.1	+0.8	OB-	(12.2)*	11.74	(0.46)*	−0.22		2.91	0.03	0.03 ± 0.05	25000	−2.9	1,24

Table 1.

Open in new tab

Basic data of 20 high-velocity post-AGB candidates.^†

								E(B − V)
Star	l (°)	b (°)	Sp.	V	G	(B − V)	(B − V)₀ Sp	Sp	SFD	3D	Adopted	T_eff (K)	B.C	Ref.^‡
(1) IRAS 02143+5852	133.8	−1.93	F7Ie	13.8	13.51	1.22	0.48	0.74	1.05		...	6000	−0.07	1,2,3
(2) IRAS 05089+0459	196.3	−19.5	M3I	14.08	13.13	1.74			0.14		...	3200	−2.24	1,4
(3) IRAS 05208−2035	222.8	−28.3		9.48	8.98	1.04	0.7:	0.3:	0.06	0.08	0.3 ± 0.2	4900	−0.33	5,6,7
(4) HD 46703	162.0	+19.	F7I	9.04	8.84	0.48	0.02	0.46	0.08	0.10	0.46 ± 0.20	6000	−0.06	1,7,8,9
(IRAS 06338+5333)
(5) HD 56126	206.7	+10.0	F5Ia	8.32	8.06	0.88	0.32	0.56	0.08	0.00	0.56 ± 0.20	6500	−0.03	1,10,11,12
(IRAS 07134+1005)
(6) IRAS 07140−2321	236.6	−5.4	F5I	10.73	10.49	0.43	0.23	0.20	0.59	0.57	0.57 ± 0.20	7000	0.0	1,13
(7) IRAS 07227−1320	228.7	+1.2	M1I	12.55	11.6	1.96	1.69	0.27	0.51	0.43	0.43 ± 0.20	3500	−1.45	1,14
(8) IRAS 08187−1905	240.6	+9.8	F6Ib/II	9.02	8.83	0.61	0.40	0.21	0.11	0.15	0.21 ± 0.05	6150	− 0.06	1,12,15
(9) HD 116745	309.1	+15.2	A7/A9e	10.79	10.68	0.29	0.13	0.16	0.13		0.16 ± 0.05	6950	−0.0	1,16
(10) IRAS 14325−6428	313.9	+4.1	F5I	12.0	11.27	0.56	0.32	0.24	0.64	0.89	0.89 ± 0.20	6400	−0.03	1,11,12
(11) IRAS 15210-6554	317.7	−7.7	K2I	11.85	11.72	(0.03)*	1.36		0.20		...	4310	−0.61	1
(12) HD 137569	21.9	+51.9	B9Iab:p	7.91	7.89	−0.05	...	0.0	0.05	0.01	0.01 ± 0.05	10500	−0.53	1,17,18
(13) BD +33 2642	52.7	+50.8	O7p	10.73	10.78	−0.12	−0.27	0.15	0.02	0.06	0.15 ± 0.05	20000	−1.66	1,19,20
(14) BD +32 2754	53.6	+41.5	F8	9.55	9.46	0.57	0.56	0.01	0.02	0.02	0.01 ± 0.05	5750	−0.09	1,14
(15) HD161796	77.1	+30.9	F3Ib	7.21	7.08	0.47	0.26	0.21	0.03	0.04	0.21 ± 0.05	6500	−0.03	1,9,12,21
(IRAS 17436+5003)
(16) BD −12 4970	018.0	+1.6	B0.5Ia	8.78	8.30	1.02	−0.21	1.23	2.71	1.58	1.23 ± 0.20	27000	−2.40	1
(17) IRAS 18075−0924	019.8	+4.7	—	13.9	12.47	1.4			1.41		...			1
(18) HD 178443	354.2	−21.5	F8	10.02	9.80	0.673	0.56	0.11	0.09		0.11 ± 0.05	5180	−0.09	1,22
(19) PHL 1580	031.3	−43.5	B0I	12.33	12.19	(0.14)*	−0.22		0.04	0.03	0.03 ± 0.05	24000	−2.8	1,23
(20) LS III +52 5	095.1	+0.8	OB-	(12.2)*	11.74	(0.46)*	−0.22		2.91	0.03	0.03 ± 0.05	25000	−2.9	1,24

								E(B − V)
Star	l (°)	b (°)	Sp.	V	G	(B − V)	(B − V)₀ Sp	Sp	SFD	3D	Adopted	T_eff (K)	B.C	Ref.^‡
(1) IRAS 02143+5852	133.8	−1.93	F7Ie	13.8	13.51	1.22	0.48	0.74	1.05		...	6000	−0.07	1,2,3
(2) IRAS 05089+0459	196.3	−19.5	M3I	14.08	13.13	1.74			0.14		...	3200	−2.24	1,4
(3) IRAS 05208−2035	222.8	−28.3		9.48	8.98	1.04	0.7:	0.3:	0.06	0.08	0.3 ± 0.2	4900	−0.33	5,6,7
(4) HD 46703	162.0	+19.	F7I	9.04	8.84	0.48	0.02	0.46	0.08	0.10	0.46 ± 0.20	6000	−0.06	1,7,8,9
(IRAS 06338+5333)
(5) HD 56126	206.7	+10.0	F5Ia	8.32	8.06	0.88	0.32	0.56	0.08	0.00	0.56 ± 0.20	6500	−0.03	1,10,11,12
(IRAS 07134+1005)
(6) IRAS 07140−2321	236.6	−5.4	F5I	10.73	10.49	0.43	0.23	0.20	0.59	0.57	0.57 ± 0.20	7000	0.0	1,13
(7) IRAS 07227−1320	228.7	+1.2	M1I	12.55	11.6	1.96	1.69	0.27	0.51	0.43	0.43 ± 0.20	3500	−1.45	1,14
(8) IRAS 08187−1905	240.6	+9.8	F6Ib/II	9.02	8.83	0.61	0.40	0.21	0.11	0.15	0.21 ± 0.05	6150	− 0.06	1,12,15
(9) HD 116745	309.1	+15.2	A7/A9e	10.79	10.68	0.29	0.13	0.16	0.13		0.16 ± 0.05	6950	−0.0	1,16
(10) IRAS 14325−6428	313.9	+4.1	F5I	12.0	11.27	0.56	0.32	0.24	0.64	0.89	0.89 ± 0.20	6400	−0.03	1,11,12
(11) IRAS 15210-6554	317.7	−7.7	K2I	11.85	11.72	(0.03)*	1.36		0.20		...	4310	−0.61	1
(12) HD 137569	21.9	+51.9	B9Iab:p	7.91	7.89	−0.05	...	0.0	0.05	0.01	0.01 ± 0.05	10500	−0.53	1,17,18
(13) BD +33 2642	52.7	+50.8	O7p	10.73	10.78	−0.12	−0.27	0.15	0.02	0.06	0.15 ± 0.05	20000	−1.66	1,19,20
(14) BD +32 2754	53.6	+41.5	F8	9.55	9.46	0.57	0.56	0.01	0.02	0.02	0.01 ± 0.05	5750	−0.09	1,14
(15) HD161796	77.1	+30.9	F3Ib	7.21	7.08	0.47	0.26	0.21	0.03	0.04	0.21 ± 0.05	6500	−0.03	1,9,12,21
(IRAS 17436+5003)
(16) BD −12 4970	018.0	+1.6	B0.5Ia	8.78	8.30	1.02	−0.21	1.23	2.71	1.58	1.23 ± 0.20	27000	−2.40	1
(17) IRAS 18075−0924	019.8	+4.7	—	13.9	12.47	1.4			1.41		...			1
(18) HD 178443	354.2	−21.5	F8	10.02	9.80	0.673	0.56	0.11	0.09		0.11 ± 0.05	5180	−0.09	1,22
(19) PHL 1580	031.3	−43.5	B0I	12.33	12.19	(0.14)*	−0.22		0.04	0.03	0.03 ± 0.05	24000	−2.8	1,23
(20) LS III +52 5	095.1	+0.8	OB-	(12.2)*	11.74	(0.46)*	−0.22		2.91	0.03	0.03 ± 0.05	25000	−2.9	1,24

†

“( )*” indicates (V − R) for (11) IRAS 15210−6554, (V − G) for (19) PHL 1580, and B mag and (B − G) for (20) LS III +52 5. E(B − V)_Sp indicates (B − V) − (B − V)₀, where (B − V)₀ is estimated from the spectral type. E(B − V)_SFD is from the 2D dust extinction map of Schlegel, Finkbeiner, and Davis (1998). E(B − V)_3D is taken from 3D dust maps of Green et al. (2018) if |b| > 10° and Chen et al. (2019) if |b| < 10°.

‡

References: 1. SIMBAD; 2. Fujii, Nakada, and Parthasarathy 2002); 3. Omont et al. (1993); 4. Iyengar and Parthasarathy (1997); 5. Gielen et al. (2011); 6. Rao, Giridhar, and Lambert (2012); 7. Oomen et al. (2018); 8. Luck and Bond (1984); 9. Parthasarathy and Pottasch (1986); 10. Parthasarathy, Garcia Lario, and Pottasch (1992); 11. De Smedt et al. (2016); 12. Kamath et al. (2022); 13. Gielen et al. (2011); 14. Vickers et al. (2015); 15. Reddy and Parthasarathy (1996); 16. Gonzalez and Wallerstein (1992); 17. Martin (2004); 18. Martin (2006); 19. Napiwotzki, Heber, and Koeppen (1994); 20. Van Winckel et al. (2014); 21. Luck et al. (1990); 22. McWilliam et al. (1995); 23. McCausland et al. (1992); 24. Hardorp, Theile, and Voigt (1964).

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