Spatially Resolved Molecular Hydrogen Emission in the Inner 200 AU Environments of Classical T Tauri Stars
We present 2.0-2.4 μm integral field spectroscopy at adaptive optics spatial resolution (∼0.1″) obtained with the Near-infrared Integral Field Spectrograph (NIFS) at Gemini North Observatory of six classical T Tauri stars: T Tau, DG Tau, XZ Tau, HL T
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|Source:||Astrophysical Journal, The|
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