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   PR # 12032
    Lynds 1551 is a small star forming cloud in the nearby Taurus-Auriga
    cloud complex. It contains $\sim$20 T Tauri stars (both classical and
    weak-lined), several embedded protostars, bipolar flows and Herbig-
    Haro objects, and one young B star.  The proposed field hasa dozen
    widely separated soft $ROSAT$ PSPC sources and was probably detected
    in 2-6 keV X-rays with $HEAO-1$.  The proposed $ASCA$ images will
    detect X-rays from deeply embedded protostars and T Tauri stars,
    confirm and study the hard X-ray component of T Tauri stars, and give
    high-resolution X-ray spectra to test multi-temperature models from
    magnetically active young stars.


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