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Bringing the Visible Universe into Focus with Robo-AO
Published on: February 12, 2013
チャンドラとXMM-ニュートンの科学の最初の10年
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
まとめ
NASAのチャンドラX線天文台とESAのXMM-ニュートンは,かつてないX線感度で天文学に革命をもたらしました. これらのミッションは,高解像度画像とエネルギー測定を提供し,宇宙X線源に関する私たちの理解を変革します.
科学分野:
- 天文学 天文学
- 天体物理学 天体物理学
- X線天文学 X線天文学
背景:
- 太陽系外X線源の最初の検出は,50年未満前に発生しました.
- NASAのチャンドラX線天文台とESAのXMM-ニュートンは10年前に打ち上げられました.
- これらの観測所は,X線天文学の感度において大きな飛躍を表しています.
研究 の 目的:
- チャンドラとXMM-ニュートンによって行われた重要な発見を強調するために.
- これらの観測所が21世紀の天文学に与える変革的な影響を紹介するためです.
- チャンドラとXMM-ニュートンの補完的な能力を強調する.
主な方法:
- 高解像度イメージング機能を活用する.
- 宇宙X線のエネルギーを正確に測定する.
- 2つの主要なX線天文台の組み合わせた力を活用する.
主要な成果:
- 400年の光学望遠鏡の進歩に匹敵する感度増加を達成しました.
- 宇宙X線源の詳細な研究を可能にしました.
- 数多くの天文学的発見を促した.
結論:
- チャンドラとXMM-ニュートンは,21世紀の天文学を根本的に変えました.
- これらの観測所の補完的な性質は,科学的リターンを最大化します.
- 継続的な観測は,X線天文学のさらなる画期的な発見を約束しています.
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