Table 1: The IRAS number, the HD number or the name from the GCVS, the spectral type, the equatorial coordinates $\alpha $ and $\delta $ (J2000), the effective temperature $T_{{\rm eff}}$, the surface gravity $\log g$, the metallicity [ Fe/ H], the reference for the model parameters, the type of object (post-AGB, RV Tauri or New Sample) and a reference where the orbital motion of the object can be found, are given. Note that IRAS 11472-0800 is a strongly depleted object added to our sample stars.
1 2 3 4 5 6 7 8 9 10 11 12
No IRAS number HD number or Spectral $\alpha $ (J2000) $\delta $ (J2000) $T_{{\rm eff}}$ $\log g$ [Fe/H] Reference Model Parameters Type Reference Binarity
    GCVS name type (h m s) ( $\hbox{$^\circ$ }~\hbox{$^\prime$ }~\hbox{$^{\prime\prime}$ }$) (K) (cgs)        
1 IRAS 04166+5719 TW Cam G3I 04 20 48.1 +57 26 26 4800 0.0 -0.5 Giridhar et al. (2000) RV Tauri  
2 IRAS 04440+2605 RV Tau G2I 04 47 06.8 +26 10 44 4500 0.0 -0.4 Giridhar et al. (2000) RV Tauri  
3 IRAS 05208-2035   M0e+F 05 22 59.423 -20 32 53.03 4000 0.5 0.0 from spectral type New Sample  
4 IRAS 06034+1354 DY Ori G0I 06 06 12.3 +13 53 09 6000 1.5 -2.0 Gonzalez et al. (1997b) RV Tauri  
5 IRAS 06072+0953 CT Ori F9I 06 09 57.4 +09 52 35 5500 1.0 -2.0 Gonzalez et al. (1997a) RV Tauri  
6 IRAS 06108+2743 SU Gem G5I 06 14 00.8 +27 42 12 5750 1.125 -0.7 Wahlgren (1992) RV Tauri  
7 IRAS 06160-1701 UY CMa G0V 06 18 16.367 -17 02 34.72 5500 1.0 0.0 from spectral type RV Tauri  
8 IRAS 06176-1036 HD 44179 F1I 06 19 58.2160 -10 38 14.691 7500 0.8 -3.3 Waelkens et al. (1992) post-AGB Van Winckel et al. (1995)
9 IRAS 06338+5333 HD 46703 F3I 06 37 52.4253 +53 31 01.957 6250 1.0 -1.5 from spectrum post-AGB Hrivnak, private communication
10 IRAS 06472-3713 ST Pup F7I 06 48 56.4131 -37 16 33.332 5750 0.5 -1.5 Gonzalez & Wallerstein (1996) RV Tauri Gonzalez & Wallerstein (1996)
11 IRAS 07008+1050 HD 52961 F6I 07 03 39.6314 +10 46 13.067 6000 0.5 -4.8 Waelkens et al. (1991b) post-AGB Waelkens et al. (1992)
12 IRAS 07140-2321 SAO 173329 F5I 07 16 08.271 -23 27 01.61 7000 1.5 -0.8 Van Winckel (1997) post-AGB Van Winckel et al. (1995)
13 IRAS 07284-0940 U Mon G0I 07 30 47.5 -09 46 37 5000 0.0 -0.8 Giridhar et al. (2000) RV Tauri Pollard & Cottrell (1995)
14 IRAS 08011-3627 AR Pup F0I 08 03 01.1 -36 35 47 6000 1.5 -1.0 Gonzalez et al. (1997b) RV Tauri  
15 IRAS 08544-4431   F3 08 56 14.182 -44 43 10.73 7250 1.5 -0.5 Maas et al. (2003) New Sample Maas et al. (2003)
16 IRAS 09060-2807   F5 09 08 10.1 -28 19 10 6500 1.5 -0.5 Maas et al. (2005) New Sample  
17 IRAS 09144-4933   G0 09 16 09.1 -49 46 06 5750 0.5 -0.5 Maas et al. (2005) New Sample  
18 IRAS 09256-6324 IW Car F7I 09 26 53.4 -63 37 48 6700 2.0 -1.0 Giridhar et al. (1994) RV Tauri  
19 IRAS 09400-4733   M0 09 41 52.9 -47 47 03         New Sample  
20 IRAS 09538-7622   G0 09 53 58.5 -76 36 53 5500 1.0 -0.5 Maas et al. (2005) New Sample  
21 IRAS 10158-2844 HR 4049 A6I 10 18 07.5903 -28 59 31.201 7500 1.0 -4.5 Dominik et al. (2003) post-AGB Waelkens et al. (1991b)
22 IRAS 10174-5704   K:rr 10 19 18.1 -57 19 36         New Sample  
23 IRAS 10456-5712 HD 93662 K5 10 47 38.3965 -57 28 02.679 4250 0.5 0.0 from spectral type New Sample  
24 IRAS 11000-6153 HD 95767 F0I 11 02 04.314 -62 09 42.84 7600 2.0 0.1 Van Winckel (1997) post-AGB Van Winckel et al. (1995)
25 IRAS 11118-5726 GK Car M0I 11 14 01.3 -57 43 09         RV Tauri  
26 IRAS 11472-0800   F5I 11 49 48.5 -08 17 21 5750 1.0 -2.5 from spectrum    
27 IRAS 12067-4508 RU Cen F6I 12 09 23.7 -45 25 35 6000 1.5 -2.0 Maas et al. (2002) RV Tauri  
28 IRAS 12185-4856 SX Cen G3V 12 21 12.6 -49 12 41 6000 1.0 -1.0 Maas et al. (2002) RV Tauri Maas et al. (2002)
29 IRAS 12222-4652 HD 108015 F3Ib 12 24 53.501 -47 09 07.51 7000 1.5 -0.1 Van Winckel (1997) post-AGB  
30 IRAS 13258-8103   G5 De 13 31 07.1 -81 18 30         New Sample  
31   EN TrA F2Ib 14 57 00.6847 -68 50 22.879 6000 1.0 -0.5 Van Winckel (1997) RV Tauri Van Winckel et al. (1995)
32 IRAS 15469-5311   F3 15 50 44.0 -53 20 44 7500 1.5 0.0 Maas et al. (2005) New Sample  
33 IRAS 15556-5444   F8 15 59 32.1 -54 53 18         New Sample  
34 IRAS 16230-3410   F8 16 26 20.29 -34 17 12.3 6250 1.0 -0.5 Maas et al. (2005) New Sample  
35 IRAS 17038-4815   G2p(R)e 17 07 36.3 -48 19 08 4750 0.5 -1.5 Maas et al. (2005) New Sample  
36 IRAS 17233-4330   G0p(R) 17 26 57.5 -43 33 13 6250 1.5 -1.0 Maas et al. (2005) New Sample  
37 IRAS 17243-4348 LR Sco G2 17 27 56.1 -43 50 48 6250 0.5 0.0 Maas et al. (2005) New Sample  
38 IRAS 17534+2603 89 Her F3I 17 55 25.1889 +26 02 59.966 6500 1.0 0.0 Waters et al. (1993) post-AGB Waters et al. (1993)
39 IRAS 17530-3348 AI Sco G4I 17 56 18.5 -33 48 47 5000 0.0 0.0 from spectrum RV Tauri  
40 IRAS 18123+0511   G5 18 14 49.4 +05 12 55 5000 0.5 0.0 from spectral type New Sample  
41 IRAS 18158-3445   F6 18 19 13.6 -34 44 32 6500 1.5 0.0 from spectral type New Sample  
42 IRAS 18281+2149 AC Her F4I 18 30 16.2 +21 52 00 5500 0.5 -1.5 Van Winckel et al. (1998) RV Tauri Van Winckel et al. (1998)
43 IRAS 18564-0814 AD Aql G8I 18 59 08.1 -08 10 14 6300 1.25 -2.1 Giridhar et al. (1998) RV Tauri  
44 IRAS 19125+0343   F2 19 15 00.8 +03 48 41 7750 1.0 -0.5 Maas et al. (2005) New Sample  
45 IRAS 19163+2745 EP Lyr A4I 19 18 17.5 +27 50 38 7000 2.0 -1.5 Gonzalez et al. (1997b) RV Tauri  
46 IRAS 19157-0247   F3 19 18 22.5 -02 42 09 7750 1.0 0.0 Maas et al. (2005) New Sample  
47 IRAS 20056+1834 QY Sge G0 De 20 07 54.8 +18 42 57 5850 0.7 -0.4 Rao et al. (2002) New Sample  
48 IRAS 20117+1634 R Sge G0I 20 14 03.8 +16 43 35 5750 0.0 -0.5 Gonzalez et al. (1997b) RV Tauri  
49 IRAS 20343+2625 V Vul G8I 20 36 31.8 +26 36 17 5250 1.0 0.0 from spectral type RV Tauri  
50 IRAS 22327-1731 HD 213985 A2I 22 35 27.5259 -17 15 26.889 8250 1.5 -1.0 from spectrum post-AGB Van Winckel et al. (1995)
51   BD+39$^{\circ }$4926 A9I 22 46 11.2273 +40 06 26.294 7500 1.2 -2.9 Van Winckel et al. (1995) post-AGB Kodaira et al. (1970)


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