NIR spectra of SN 2014C 1-5yr post-explosion
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Supernova (SN) 2014C is unique: a seemingly typical hydrogen-poor SN that started to interact with a dense, hydrogen-rich circumstellar medium (CSM) ~100 days post-explosion....
超新星（Supernova, SN）2014C极具特殊性：它是一颗看似典型的贫氢超新星，却在爆炸后约100天时开始与致密的富氢星周介质（circumstellar medium, CSM）发生相互作用……
