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Echo Particle Image Velocimetry
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来自1843年埃塔卡里奈火山喷发的冲击波
1Astronomy Department, University of California, 601 Campbell Hall, Berkeley, California 94720-3411, USA. nathans@astro.berkeley.edu
Nature
|September 12, 2008
概括
观测显示,埃塔卡里纳在19世纪喷发时喷出的物质极为快,其动能增加了一倍. 这表明,强大的超新星式爆炸,而不仅仅是恒星风,可能为发光蓝变量 (LBV) 喷发提供动力.
科学领域:
- 天文学 天文学
- 天体物理学 天体物理学
- 恒星进化 恒星进化
背景情况:
- 在超新星发生之前,大质量恒星会以发光蓝色变量 (LBVs) 的形式发生激烈的喷发.
- 目前尚不清楚LBV爆发的原因.
- 埃塔卡里纳在19世纪爆发时,它以650公里/秒的速度抛出了12个太阳质量,其动能为1050 erg.
研究的目的:
- 为了研究19世纪埃塔卡里纳喷发的喷射物完全分布和速度.
- 为了确定LBV喷发的能量来源和影响.
主要方法:
- 观测天文学是一种观测天文学.
- 分析来自eta Carinae的高速喷射物.
主要成果:
- 在19世纪的事件中发现了更快的物质 (3,5006,000公里/秒) 弹出.
- 这种快速的物质使喷发的动能增加了一倍,产生了冲击波.
- 埃塔卡里奈的外现在类似于低能超新星残余物.
结论:
- 像Eta Carinae这样的LBV喷发可能是由与超新星竞争的深层爆炸驱动的.
- 脉冲对的不稳定性可以触发如此强大的LBV事件.
- 这一发现可能会改变对类似银河系外事件的解释.
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