V.P. Ivanov 1*, D.P. Kjurkchieva1, M. Srinivasa
Rao2
Abstract.
We propose a procedure for light-curve solutions of eclipsing
binary stars in the Small Magellanic Cloud (SMC) for which photometric
data have been obtained in the framework of the OGLE project. We also
present a way of determining the global stellar parameters on
the basis of the obtained solutions, some empirical relations as
well as the distance to the SMC. Several examples illustrate this
procedure.
Keywords: stars: binaries: eclipsing - stars: fundamental
parameters - stars: general - galaxies: individual: SMC
1 Department of Physics, Shumen University, 9700 Shumen,
Bulgaria
2 Indian Institute of Astrophysics, Bangalore 560034, India