Table 8: Parameters of interstellar polarization ( $P_{\rm is}$; $\theta _{\rm is}$) derived by the "field star method'' and values of intrinsic polarization ($P_{\ast }$; $\theta _{\ast }$) of programme stars.
  RU Cen SX Cen UW Cen DY Cen  
D (kpc) 2.0 4.0 2.5 5.2 2.8 3.3 5.0  
$P_{\rm is}$; $\theta _{\rm is}$ 1.0% ; $85^\circ$ 1.5% ; $85^\circ$ 1.3% ; $85^\circ$ 1.8% ; $80^\circ$ 1.4% ; $83^\circ$ 1.5% ; $80^\circ$ 2.0% ; $80^\circ$  
$P_{\ast }$; $\theta _{\ast }$ 1.5% ; $15^\circ$ 1.7% ;  $8^\circ$ 1.0% ; $3^\circ$ 1.4% ; $173^\circ$ 1.0% ; $^\ast$ 1.1% ;  $^\ast$ 2.0% ; $158^\circ$  
  V1711 Sgr DS Aqr UY Ara RY Sgr

D (kpc)		 0.5 1.0 0.47 3.0 10 3-5 2.0
$P_{\rm is}$; $\theta _{\rm is}$ 0.5% ; $5^\circ$ 0.8% ; $15^\circ$ 0.05% ; $140^\circ$ 0.2% ; $120^\circ$ 1.5% ;  $35^\circ$ 2.0% ;  $55^\circ$ $0.90\pm0.12$% ; $82^\circ$
$P_{\ast }$; $\theta _{\ast }$ 0.55% ; $65^\circ$ 0.6% ; $85^\circ$ 0.26% ;  $74^\circ$ 0.25% ; $168^\circ$ 1.0% ; $103^\circ$ 1.0% ; $145^\circ$ 1.0% ; $170^\circ$
  R Sct AI Sco BU Cen R Sge  

D (kpc)		 0.43 3.0 1.5 3.0 3.0  
$P_{\rm is}$; $\theta _{\rm is}$ $0.65\pm0.05$% ; $50^\circ\pm5^\circ$ $1.8\pm0.2$% ; $5^\circ$ 0.9% ; $70^\circ$ 1.4% ; $80^\circ$ 1.8% ;  $30^\circ$  
$P_{\ast }$; $\theta _{\ast }$ 0.63% ; $18^\circ$ 0.9% ; $120^\circ$ 1.0% ; $150^\circ$ 1.2% ; $163^\circ$ 1.5% ; $213^\circ$  
$^\ast$ For two measurements on JD6991 and JD7000, the values of  $\theta _{\ast }$ differ significantly: $\approx$$140^\circ$ and $\approx$$5^\circ$ respectively.

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