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Bringing the Visible Universe into Focus with Robo-AO
Published on: February 12, 2013
科学的第一个十年与钱德拉和XMM-牛顿的科学
Maria Santos-Lleo1, Norbert Schartel, Harvey Tananbaum
1XMM-Newton Science Operations Centre, European Space Agency, Villanueva de la Cañada, 28691 Madrid, Spain.
Nature
|December 25, 2009
概括
美国宇航局的钱德拉X射线天文台和欧洲航天局的XMM-牛顿已经用前所未有的X射线灵敏度彻底改变了天文学. 这些任务提供了高分辨率图像和能量测量,改变了我们对宇宙X射线源的理解.
科学领域:
- 天文学 天文学
- 天体物理学 天体物理学
- X射线天文学X射线天文学
背景情况:
- 太阳系外X射线源的首次检测发生在不到50年前.
- 美国宇航局的钱德拉X射线天文台和欧洲航天局的XMM-牛顿在十年前发射.
- 这些天文台代表了X射线天文学灵敏度的重大飞跃.
研究的目的:
- 为了强调钱德拉和XMM-牛顿所做的关键发现.
- 展示这些天文台对21世纪天文学的影响.
- 为了强调Chandra和XMM-Newton的互补能力.
主要方法:
- 使用高分辨率成像能力.
- 精确测量宇宙X射线的能量.
- 利用两个主要的X射线天文台的联合力量.
主要成果:
- 实现了与400年光学望远镜进步相提并论的灵敏度增加.
- 能够对宇宙X射线源进行详细研究.
- 促进了众多的天文学发现.
结论:
- 钱德拉和XMM-牛顿从根本上改变了21世纪的天文学.
- 这些天文台的互补性质最大限度地提高了科学回报.
- 持续的观测有望在X射线天文学领域进一步突破性发现.
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