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Table 1

Binary post-AGB stars in our interferometric survey.

Nr. IRAS Name α2000 δ2000 Spectral Pbinary a1 sin(i) f(M) RVb Ref.
[h m s] [  o  ’  ”] type [days] [AU] [M]

1 04440+2605 RV Tau 04 47 06.7 +26 10 45.6 K3pv 1180 ± 15 y Zsoldos (1996)
2 07008+1050 HD 52961 07 03 39.6 +10 46 13.1 F6I 1297 ± 7 1.54 0.29 y Van Winckel et al. (1999)
3 07284-0940 U Mon 07 30 47.5 09 46 36.8 K0IIb ~2600 y Pollard et al. (2006)
4 08011-3627 AR Pup 08 03 01.6 36 35 47.9 F0I 1250 ± 300 y Kiss et al. (2007)
5 08544-4431 08 56 14.2 44 43 10.7 F3 508 ± 2 0.39 0.03 Maas et al. (2003)
6 09256-6324 IW Car 09 26 53.3 63 37 48.9 F7I ~1440 y Pollard et al. (1996)
7 10158-2844 HR 4049 10 18 07.6 28 59 31.2 A4Ib/II 434 ± 1 0.61 0.16 y Waelkens et al. (1991a)
8 10174-5704 10 19 16.9 57 19 26.0 323 ± 50 0.17 0.007 Maas (2003)
9 10456-5712 HD 93662 10 47 38.4 57 28 02.7 K5 572 ± 6 0.015 1.4 × 10-6 Maas (2003)
10 11385-5517 HD 101584 11 40 58.8 55 34 25.8 A6Ia 218 ± 1 a y Bakker et al. (1996)
11 12185-4856 SX Cen 12 21 12.6 49 12 41.1 G3V 592 ± 13 1.23 0.70 y Deroo et al. (2006)
12 12222-4652 HD 108015 12 24 53.5 47 09 07.5v F4Ib/II 914 ± 4 0.29 0.004 van Winckel et al. (2009)
13 15469-5311 15 50 43.8 53 20 43.3 F3 390 ± 1 0.42 0.07 van Winckel et al. (2009)
14 17038-4815 17 07 36.6 48 19 08.6 G2p 1386 ± 12 1.5 0.22 y Manick et al. (2017)
15 17243-4348 LR Sco 17 27 53.6 43 50 46.3 G2 ~475 Maas (2003)
16 17534+2603 89 Her 17 55 25.2 +26 03 00.0 F3 288 ± 1 0.08 8 × 10-4 Waters et al. (1993)
17 18281+2149 AC Her 18 30 16.2 +21 52 00.6 F2Iep 1194 ± 6 1.39 0.25 Van Winckel et al. (1998)
18 19125+0343 19 15 01.2 +03 48 42.7 F2 520 ± 2 0.58 0.097 van Winckel et al. (2009)
19 22327-1731 HD 213985 22 35 27.5 17 15 26.9 A0III 258.6 ± 0.3 0.79 0.97 y Waelkens et al. (1995)

Notes. We give the coordinates together with the spectral type retrieved from Simbad. Most objects are confirmed binaries and some orbital parameters (orbital period, semi-major axis asin(i), and mass function f(M)) are provided. We note for which targets the photometric “RVb” phenomenon has been reported.

(a)

Díaz et al. (2007) reported a period of 144 d on an IAU symposium.

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