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星系外流中的恒星形成
R Maiolino1,2, H R Russell3, A C Fabian3
1Cavendish Laboratory, University of Cambridge, 19 J. J. Thomson Avenue, Cambridge CB3 0HE, UK.
Nature
|March 28, 2017
概括
我们发现了巨大的星系外流中恒星形成的第一证据. 这一发现表明恒星形成的新模式可能会影响银河系的进化,
科学领域:
- 天文学与天体物理学
- 银河系的演变
- 恒星形成
背景情况:
- 巨大的星系外流具有有利于恒星形成的条件.
- 模型预测出流中的恒星形成,影响银河系形态和恒星群.
- 目前还没有观察到外流中恒星形成的证据.
研究的目的:
- 在星系外流中提供明确的恒星形成观测证据.
- 研究这种恒星形成模式对星系进化和化学丰富的潜在影响.
主要方法:
- 在红移0.0448的星系外流的光谱观测.
- 分析光谱数据以确定正在进行的恒星形成的信号.
主要成果:
- 在观测到的星系外流中明确检测到恒星形成.
- 在外流中推断的恒星形成速度超过每年15个太阳质量.
- 这表明以前的观察可能错过了类似的现象,
结论:
- 在银河系外流中可能发生恒星形成, 挑战以前的假设.
- 这种恒星形成方式可能在银河系进化和环银河系和星际介质的化学丰富中发挥着重要作用.
- 需要进一步的观测和适当的诊断来评估星系外流中恒星形成的普遍性.
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