OI equivalent widths in Be stars
收藏B2FIND2026-04-04 收录
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https://b2find.eudat.eu/dataset/e9595d51-c250-5ea4-b45e-6f87d57a6327
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The possibility of the Ly{beta} fluorescence mechanism being operational in classical Be (CBe) stars and thereby contributing to the strength of the OI{lambda}8446 line has been...
