Coulour-Period relation for Cepheids
收藏B2FIND2026-03-19 收录
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https://b2find.eudat.eu/dataset/b1bdbafd-ef7a-5106-b7a4-b10197b23220
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We compare mid-infrared (IR) 3.6 and 4.5{mu}m Warm Spitzer observations for Cepheids in the Milky Way and the Large and Small Magellanic Clouds. Using models, we explore in...



