I present low-resolution optical spectroscopy of two very low luminosity young stellar object candidates in Taurus. Both have faint companions with separations less than 6'', reported by Itoh, Tamura, & Nakajima, who considered them as likely substellar objects. However, the optical spectra demonstrate that they are reddened background stars (Av ≥ 4 mag). One of the candidate primaries is confirmed as a new member of the Taurus T Tauri association. It is a classical T Tauri star of early M spectral type with blue and near-infrared continuum excesses. The spectrophotometric properties indicate that it could be an edge-on disk. The other candidate primary is a background early-type star.
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机译：我介绍了金牛座中两个非常低亮度的年轻恒星候选物的低分辨率光谱学。 Itoh，Tamura和Nakajima报道说，他们俩都有间隔小于6英寸的昏暗伴侣，他们认为它们很可能是亚星体。但是，光谱表明它们是变红的背景星（Av≥4 mag）。候选候选人之一被确认为Taurus T Tauri协会的新成员。它是早期M光谱类型的经典T Tauri星，具有蓝色和近红外连续谱过量。分光光度特性表明它可能是边缘光盘。另一个候选主要对象是背景早期型恒星。
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