超过一半的远红外背景光来自z >or= 1.2的星系
Mark J Devlin1, Peter A R Ade, Itziar Aretxaga
1Department of Physics & Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, Pennsylvania 19104, USA. devlin@physics.upenn.edu
Nature
|April 11, 2009
概括
亚毫米调查显示,大部分远红外背景 (FIRB) 来自发光,高红移星系. 这些尘埃星爆星系,在z>1.2中观察到,是这种宇宙辐射的主要贡献者.
科学领域:
- 银河系外天文学 银河系外天文学
- 宇宙尘埃研究 宇宙尘埃研究
- 银河系的进化 银河系的进化
背景情况:
- 毫米以下的调查已经确定了发光,高红移,灰尘的星爆星系.
- 这些星系的恒星形成速度是本地宇宙的数百倍.
- 恒星光被尘埃吸收,并在远红外线中重新辐射,为宇宙背景做出贡献.
研究的目的:
- 将综合远红外背景 (FIRB) 分解为来自单个星系的贡献.
- 为了研究超银河系背景辐射在亚毫米波长的来源.
- 为了确定FIRB发射星系的红移分布.
主要方法:
- 在250,350和500微米进行了银河系外调查.
- 将新的500微米数据与现有的24微米观测数据结合起来.
- 分析了光谱能量分布和红移信息.
主要成果:
- 所有远红外背景 (FIRB) 都归因于单个星系.
- 红移z >or= 1.2的星系占FIRB的70%.
- 在z > 1处的超发光星系在最长波长 (500微米) 的信号中占据主导地位.
结论:
- FIRB主要是由高红移,尘土星爆星系产生的.
- 在z > 1处的星系数量对于了解早期宇宙的能量预算至关重要.
- 已解决的单个星系解释了整个观察到的FIRB.
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