在银河系中心区域的红外扩散星际波段
T R Geballe1, F Najarro, D F Figer
1Gemini Observatory, 670 N. A'ohoku Place, Hilo, Hawaii 96720, USA. tgeballe@gemini.edu
Nature
|November 4, 2011
概括
研究人员在银河系中心发现了13个新的分散星际波段 (DIB). 这些宇宙吸收特征,可能是基于碳的分子,出现在比以前观察到的DIB更恶劣的环境中.
科学领域:
- 天文学 天文学
- 天体物理学 天体物理学
- 频谱学是一种光谱学.
背景情况:
- 分散星际带 (DIBs) 是由于星际物质而在恒星光谱中观察到的吸收特征.
- 已知有500多个DIB,主要是在可见和近红外波长.
- 怀疑DIBs的载体是多原子含碳分子,但没有一个被确定的.
研究的目的:
- 在更长的红外波长 (1.5-1.8微米) 中寻找和描述新的DIB.
- 调查这些新发现的DIBs的起源和环境.
- 将银河系中心的DIB属性与其他扩散云的DIB属性进行比较.
主要方法:
- 高分辨率的光谱观测恒星的高灭绝向银河系中心.
- 在1.5-1.8微米波长区间分析光谱.
- 将DIB强度与星际灭绝值进行比较.
主要成果:
- 在1.5-1.8微米范围内发现了13个新的扩散星际带.
- 这些DIB主要观察到银河系中心,这表明它们起源于该地区.
- 这些DIB的相对强度与星际灭绝相关,类似于以前已知的DIB.
结论:
- 银河系中心拥有以前未知的分散星际波段,起源于一个更温暖,更恶劣的环境.
- 这些新的DIB的载体可能与已知DIB的载体相似,可能是多原子碳分子.
- DIB强度通常随着分散的星际物质的数量而变大,无论具体的环境如何.
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