Quantitative near-IR diagnostics based on equivalent widths and band ratios distinguish FUOr disks from normal late-type stars using spectra of 28 known objects.
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Quantitative Spectroscopic Diagnostics for FU Orionis-Type Young Stellar Objects
Quantitative near-IR diagnostics based on equivalent widths and band ratios distinguish FUOr disks from normal late-type stars using spectra of 28 known objects.