PHYSICAL PROPERTIES OF THE LOW-MASS ECLIPSING BINARY NSVS 02502726
PHYSICAL PROPERTIES OF THE LOW-MASS ECLIPSING BINARY NSVS 02502726
NSVS 02502726 has been known as a double-lined, detached eclipsing binary that consists of two low-mass stars. We obtained $BVRI$ photometric follow-up observations in 2009 and 2011 to measure improved physical properties of the binary star. Each set of light curves, including the 2008 data given by \cCakirli et al., …