Age Determinations of Early-M Type Pre-Main Sequence Stars Using a High-Resolution Near-Infrared Spectroscopic Method
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概要
- 論文の詳細を見る
- 2011-06-25
著者
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SUGITANI Koji
Graduate School of Natural Sciences, Nagoya City University
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ITOH Yoichi
Graduate School of Science and Technology, Kobe University
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Itoh Yoichi
Graduate School Of Engineering Division Of Materials Science And Engineering Hokkaido University
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Sugitani K
Graduate School Of Natural Science Nagoya City University
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Ita Yoshifusa
National Astronomical Observatory Of Japan
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Ita Yoshifusa
Institute Of Astronomy School Of Science The University Of Tokyo
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OASA Yumiko
University of Tokyo
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Oasa Yumiko
Department Of Education Saitama University
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Oasa Yumiko
Faculty Of Education Saitama University
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Itoh Y
Graduate School Of Science And Technology Kobe University
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Itoh Yoichi
Department Of Astronomy School Of Sciences
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Sugiyasu Kei
Department Of Astronomy Faculty Of Science Kyoto University
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Itoh Yoichi
Kobe Univ. Kobe
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TAKAGI Yuhei
Graduate School of Science, Kobe University
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Itoh Yoichi
Kobe Univ. Hyogo
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Takagi Yuhei
Graduate School Of Science Kobe University
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Ita Yoshifusa
Department Of Earth And Space Science Graduate School Of Science Osaka University
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