[C ii] 158-μm发射来自受阻莱曼-阿尔法系统的主体星系
Marcel Neeleman1, Nissim Kanekar2, J Xavier Prochaska3
1University of California Observatories-Lick Observatory, University of California, Santa Cruz, CA 95064, USA. marcel@ucsc.edu.
概括
天文学家检测到来自高红移吸收的星系的[C ii]线和尘埃辐射. 这些星系类似于巨大的恒星形成系统,
科学领域:
- 天文学与天体物理学
- 宇宙学
背景情况:
- 研究高红移星系周围的气体对于理解宇宙进化至关重要.
- 与背景类星体相比,这些星系的观测具有挑战性.
研究的目的:
- 识别和描述具有高红移 (z ~ 4) 的吸收线系统的星系.
- 研究这些星系及其周围气体的物理性质.
主要方法:
- 使用阿塔卡马大毫米/亚毫米阵列 (ALMA).
- 检测[C ii]158μm线和尘埃连续性的排放.
主要成果:
- 成功检测到两个星系在z~4的[Cii]和尘埃连续辐射.
- 这些星系与高金属性吸收系统有关.
- 宿主星系表现出与巨大的恒星形成星系相似的特性.
结论:
- 这项研究证实了超越这些星系的星际环境的缩中性气体储备.
- 这为早期星系的环银河系介质提供了新的见解.
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