超发光的超新星:不同的升起时间解释了不同的光谱
1Astrophysics Research Centre, School of Mathematics and Physics, Queen's University Belfast, Belfast, BT7 1NN UK.
概括
第一种类型的超发光超新星 (SLSNe) 呈现出多样化的光谱,但这种多样性是由喷射温度解释的,而不是祖先的差异. 一个新的诊断方法将光曲线上升时间与光谱特征联系起来,支持这些明亮爆炸的中央发动机模型.
科学领域:
- 天文学和天体物理学
- 太空爆炸 太空爆炸
- 恒星进化 恒星进化
背景情况:
- 第一种类型的超光超新星 (SLSNe) 是非常明亮的,巨大的恒星爆炸.
- 它们的光谱经常显示电离氧吸收,但亚型仍在争论中.
- 光度特性表明连续分布,与一些光谱学发现形成鲜明对比.
研究的目的:
- 为了调查I型SLSNe的光谱多样性的原因.
- 为了确定观察到的光谱亚型是否代表了根本差异或环境因素.
- 开发一种新的诊断工具,以了解SLSNe.
主要方法:
- 在接近最大光线时,对I型SLSN,PTF12dam的光谱演变进行分析.
- 开发一个亮度-时间尺度-温度-半径 (BTTR) 图.
- 创建一个简单的玩具模型用于光球速度进化.
主要成果:
- PTF12dam表现出不断变化的O II吸收概况,在拟议的亚型之间进行过渡.
- 光谱的多样性与最大光度的喷射温度有关,而不是祖先变化.
- BTTR图和玩具模型显示光曲线上升时间 (与抛出质量相关) 解释光谱和速度差异.
- SLSN的速度分布表明一个平坦的喷射密度配置,与中央发动机一致.
结论:
- I型SLSNe的光谱多样性主要是由最大光线下的喷射温度驱动的.
- 光曲线上升的持续时间是影响光谱特征和速度演变的关键因素.
- 一个中央发动机模型是最受欢迎的解释观察到的喷射物密度配置文件在SLSNe.
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