SNe 2021acya, 2021adxl, 2022qml, and 2022wed
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At late stages, massive stars experience strong mass-loss rates, losing their external layers and thus producing a dense H-rich circumstellar medium (CSM). After the explosion...
演化晚期的大质量恒星会经历强烈的质量损失过程，抛散自身外层物质，进而形成富氢致密星周介质（circumstellar medium，CSM）。恒星爆发之后……
