The origin of the local bubble

被引:99
作者
Maíz-Apellániz, J [1 ]
机构
[1] Space Telescope Sci Inst, Baltimore, MD 21218 USA
基金
美国国家航空航天局;
关键词
ISM : bubbles; ISM : structure; open clusters and associations : individual (Scorpius-Centaurus Association); solar neighborhood; stars : distances; supernovae : individual (Scorpius-Centaurus Association);
D O I
10.1086/324016
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Sun is located in a low-density region of the interstellar medium partially filled with hot gas that is the likely result of several nearby supernova explosions within the last 10 Myr. Here we use astrometric data to show that part of the Scorpius-Centaurus OB association was located closer to the present position of the Sun 5-7 Myr ago than today. Evolutionary synthesis models indicate that the association must have experienced similar to0 supernova explosions in the last 10-12 Myr, a prediction that is supported by the detection of four or five runaway stars escaping from it. The approximately six supernovae produced by the Lower Centaurus Crux subgroup are likely responsible for the creation of the Local Bubble.
引用
收藏
页码:L83 / L86
页数:4
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