在原恒星爆发期间拍摄水雪线
Lucas A Cieza1,2, Simon Casassus2,3, John Tobin4
1Núcleo de Astronomía, Facultad de Ingeniería, Universidad Diego Portales, Av. Ejercito 441, Santiago 8370191, Chile.
Nature
|July 15, 2016
概括
天文学家首次拍摄了原行星盘中的水雪线,揭示了原恒星爆发期间的动态运动. 这一发现影响了行星形成和磁盘演变的模型.
科学领域:
- 天文学与天体物理学
- 星球科学
背景情况:
- 在原行星盘中挥发性物质凝结的雪线对于颗粒生长和行星形成至关重要.
- 已观察到一氧化碳雪线,但水雪线对于小行星和巨行星核心形成至关重要,通常离恒星太近,无法看到.
研究的目的:
- 在原行星盘中描绘和描述水雪线.
- 研究原恒星爆发对雪线动态和磁盘演变的影响.
主要方法:
- 在爆发的原星V883 Ori周围的原行星盘的高分辨率成像.
- 对磁盘的强度断裂和光谱行为进行分析,以确定水雪线.
主要成果:
- 在大约42天文单位 (au) 检测到强度断裂,表明水雪线的位置.
- 在爆发期间升高的磁盘温度将水雪线推向外面.
- 频谱分析证实了由于颗粒生长受阻而增加的颗粒数密度和超越雪线的光学深度.
结论:
- 水雪线的位置非常动态,并且可以受到原星爆发的显著影响.
- 这些发现需要将动态雪线纳入磁盘进化和行星形成模型.
- 观察到的现象为彗星和巨行星形成所需的条件提供了关键的见解.
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