FUor masses inferred from Keplerian line broadening in H-band spectra match the solar neighborhood IMF, indicating a universal eruptive phase during star formation.
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High-resolution NIR spectra of 15 FUors reveal double-peaked Keplerian profiles in five K-band targets that fit disk models, J-K band correlations without clear wavelength linewidth trends, and M-band CO lines of distinct origin likely due to blending or winds.
citing papers explorer
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The FUor Mass Distribution Matches the Solar Neighborhood IMF: Evidence for a Universal Eruptive Phase
FUor masses inferred from Keplerian line broadening in H-band spectra match the solar neighborhood IMF, indicating a universal eruptive phase during star formation.
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Probing the kinematics of FU Orionis objects through high-resolution near-infrared spectroscopy
High-resolution NIR spectra of 15 FUors reveal double-peaked Keplerian profiles in five K-band targets that fit disk models, J-K band correlations without clear wavelength linewidth trends, and M-band CO lines of distinct origin likely due to blending or winds.