Abstract:Abstract.One of the handful of known PMS eclipsing binaries is a component of the spectroscopic triple TY CrA. Its secondary component is particularly interesting since it is a star of relatively high mass (1.64 M ) which is still on the pre-main sequence. The eclipsing binary was analyzed in the optical wavelength range ∼10 years ago, however, the crucial secondary eclipse minimum is very shallow. Therefore, we are obtaining new photometry in both optical and near-IR bands. We present first observations in (B… Show more
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