Distance to the SMC from eclipsing binaries
  The preliminary distance to a long period eclipsing binary in the Small
Magellanic Cloud SMC108.1.14904 is presented. The binary system contains two
non-active G-type bright giants. The orbital period is 185 days and the orbit
is circular. Using surface brightness calibration we calculated distance
modulus to the system (m-M)= 19.02 +/- 0.04 (stat.) +/- 0.05 (syst.) mag, where
systematic error is dominated by uncertainty of surface brightness calibration.
This is a second eclipsing binary in the SMC analysed by our team.
