We present phase-resolved spectroscopy of the bright, eclipsing polar HU Aqr\nobtained with high time (~30sec) and spectral (1.6 A) resolution when the\nsystem was in a high accretion state. The trailed spectrograms reveal clearly\nthe presence of three different line components with ...
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Results. We report the presence of two substellar companions to the K giant stars τ Gem and 91 Aqr. The brown dwarf orbiting τ Gem has an orbital period of 305.5±0.1 days, a minimum mass of 20.6 MJ, and an eccentricity of 0.031±0.009. The planet orbiting 91 Aqr has an orbital ...
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