Table 7: Estimates of $P_{\rm is}$ for programme stars.

Object		 l $P^{\rm is}_{1}$ b $P^{\rm is}_{2}$ E(B-V) $\overline{E(B-V)}_{\rm is}$ $P^{\rm is}_{3}$ d $P^{\rm is}_{4}$ $\overline{P}_{\rm is}$
  (deg.) (%) (deg.) (%) (Ref.)   (%) (kpc) (%) (%)

RY Sgr		 4.43 1.2 -19.45 0.5 2,6,13,14 0.12 0.6 1.3;4.0 1.8;2.1 1.1
V1711 Sgr 10.81 1.0 -27.46 0.4 7,8,9 0.12 0.6 0.43 0.8 0.7
R Sct 27.40 0.6 -1.72 ... 1,4,11,12 0.21 1.0 0.43 0.8 0.8
U Aqr 39.15 0.4 -49.81 0.3 13,14 0.03 0.3 0.16-0.93 0.4-1.5 0.3-1.3
DS Aqr 44.10 0.4 -61.56 0.2 1 0 0 0.5 0.9 0.4
R Sge 57.53 0.5 - 9.75 0.9 1,4,10 0.25 1.2 2.9-3.2 2.3 1.2
RU Cen 295.25 2.0 +16.82 0.6 1,4,5,11 0.16 0.8 1.6-3.9 2.3 1.4
SX Cen 297.87 2.0 +13.36 0.7 1,4,11 0.20 1.0 2.5-5.5 2.3-1.9 1.5
UW Cen 301.74 2.1 + 8.32 1.0 2,3,6,14 0.25 1.2 0.79;2.8-5.5 1.3;2.3-1.9 1.5
DY Cen 307.95 2.2 + 8.29 1.0 2 0.10 0.6 4.8 2.0 1.5
BU Cen 309.20 2.2 +12.41 0.7 1,4 0.20 1.0 ... ... 1.3
UY Ara 331.86 2.1 -13.78 0.7 1,11 0.17 0.8 ... ... 1.2
AI Sco 356.97 1.4 -4.45 1.8 1,5,11 0.35 1.5 2.4-3.6 2.3-2.2 1.8
(1) Goldsmith et al. (1987a); (2) Goldsmith et al. (1990); (3) Lawson & Cotterell (1990); (4) Dawson (1979); (5) Jura (1986); (6) Trimble & Kundu (1997); (7) Beers et al. (2000); (8) Fernie (1990); (9) McAlary & Welch (1986); (10) Gonzalez et al. (1997); (11) Alcolea & Bujarrabal (1991); (12) Baird & Cardelli (1985); (13) Bergeat et al. (1999); (14) Asplund et al. (1997). $P^{\rm is}_{1,2,3,4}$ calculated using Eqs. (1)-(4); $\overline{P}_{\rm is}$ is a weighted mean value of IS polarization.

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