Observational analysis reveals insights on dust and molecules in AGB stars and planetary nebulae, suggesting future research directions.
A high sensitivity and high-angular resolutions infrared space telescope, the James Webb Space Telescope (JWST) , allowed us to study dust and molecules in unprecedented details. This contribution highlights the first year of JWST ’s scientific operation, and reports prospects of dust and molecular studies in the coming future.
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M. Matsuura (2023) studied this question.
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