Photometric light curve of V1515 Cyg
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Historically, FU Orionis-type stars are low-mass, pre-main-sequence stars. The members of this class experience powerful accretion outbursts and remain in an enhanced accretion...
历史上，猎户座FU型变星（FU Orionis-type stars）属于低质量主序前星。该类天体均会经历剧烈的吸积爆发，并长期处于增强吸积状态……
