NASA Technical Reports Server (NTRS) 20050241963: Is the 21-micron Feature Observed in Some Post-AGB Stars Caused by the Interaction Between Ti Atoms and Fullerenes?

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Author:NASA Technical Reports Server (NTRS)
Language:English
File size:0.51 MB
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Similar NASA Technical Reports Server (NTRS) 20050241963: Is the 21-micron Feature Observed in Some Post-AGB Stars Caused by the Interaction Between Ti Atoms and Fullerenes?

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