Two young low-mass stars show solar C/O ratios while their inner disks are hydrocarbon-rich with C/O greater than one, providing direct evidence that disk processes enhance inner-disk carbon.
S., Gordon, I
2 Pith papers cite this work. Polarity classification is still indexing.
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2026 2verdicts
UNVERDICTED 2representative citing papers
New empirical polynomial correlations for NH3 self- and air-broadened half-widths as functions of m and K'' achieve lower mean absolute percentage errors than the current HITRAN2024 values.
citing papers explorer
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A Chemical Mismatch Between Young Stars and Their Inner Disks
Two young low-mass stars show solar C/O ratios while their inner disks are hydrocarbon-rich with C/O greater than one, providing direct evidence that disk processes enhance inner-disk carbon.
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Reassessment of ammonia self- and air-broadened half-widths in the HITRAN database
New empirical polynomial correlations for NH3 self- and air-broadened half-widths as functions of m and K'' achieve lower mean absolute percentage errors than the current HITRAN2024 values.