BL Cam light maximum times
收藏B2FIND2026-04-11 收录
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https://b2find.eudat.eu/dataset/cc36d4c0-9498-5313-8ffd-b9380d80fd6f
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Short-period high-amplitude pulsating stars of Population I (delta Sct stars) and II (SX Phe variables) exist in the lower part of the classical (Cepheid) instability strip....



