在遥远的矮星系中扩展远紫外辐射
Anshuman Borgohain1, Kanak Saha2, Bruce Elmegreen3
1Department of Physics, Tezpur University, Napaam, India. ayush.borgohain@gmail.com.
Nature
|July 21, 2022
概括
我们使用AstroSat望远镜观察蓝矮星系的恒星形成. 这表明它们的外部区域正在发生气体积聚和引力不稳定.
科学领域:
- 天文学与天体物理学
- 星系的形成和演变
背景情况:
- 蓝色紧矮星系 (BCD) 的亮度低,金属缺乏,并且集中在中心,具有恒星形成团.
- 观察BCD形成是具有挑战性的,因为在高红移时的模糊和小尺寸.
- 中间红移观测对于研究BCD的早期进化阶段至关重要,特别是受气体积累影响的外部区域.
研究的目的:
- 研究蓝矮星系的形成过程.
- 分析BCD的外部区域中的恒星形成活动.
主要方法:
- 使用阿斯特罗卫星上的紫外线成像望远镜观测GOODS南方领域的11个BCD.
- 分析远紫外线 (FUV) 辐射,并与哈勃太空望远镜的光学数据进行比较.
- 对仪表点扩散函数进行校正,以确定内在的FUV辐射轮.
主要成果:
- 在0.1-0.24红移的11个BCD的外部区域检测到过度的紫外线 (FUV) 辐射.
- 对于十个BCD,内在FUV发射的辐射形状显示出比光学对应的尺度长度更大.
- 凸起的FUV结构表明外盘的引力不稳定性.
结论:
- 浅浅的FUV形状表明宇宙积聚盘中的恒星形成有所扩大.
- 外部FUV磁盘的引力不稳定性通过动态摩擦驱动团块向内移动.
- 由于气体积聚和内部动态, BCD 外部区域正在积极演变.
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