CIT 6 and IRC+10216 30-50GHz spectra
收藏B2FIND2026-03-19 收录
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https://b2find.eudat.eu/dataset/836b4ea4-4321-5969-85d9-3eb15270239f
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At the end of the long H-burning phase (main sequence), low-to intermediate- mass stars evolve into asymptotic giant branch (AGB) stars that can have carbon-rich envelopes...
