Water Vapor in AGB Stars
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概要
- 論文の詳細を見る
Structure of the extended atmosphere in AGB stars has been investigated by analyzingH2O bands in the near-infrared region. Based on simple model analysis, we concluded that the time variation in the H2O bands with the variability phase can be attributed to the variation in the physical structure of the extended atmosphere, possibly caused by the shocks in the inner region. High wavelength/spatial resolution observations are crucial for further investigation of thestructure.
- 宇宙航空研究開発機構の論文
著者
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Takashi Onaka
Department Of Astronomy University Of Tokyo
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Takashi Onaka
Department Of Astronomy School Of Science University Of Tokyo
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Issei Yamamura
The Institute Of Space And Astronautical Science(isas)
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Mikako Matsuura
Department Of Astronomy School Of Science University Of Tokyo
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Issei YAMAMURA
Institute of Space and Astronautical Science
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Hiroshi MURAKAMI
Institute of Space and Astronautical Science
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Hiroshi Murakami
The Institute Of Space And Astronautical Science(isas)
関連論文
- Infrared Camera (IRC) onboard ASTRO-F (IRIS)
- Simulations of Observations with the Far-Infrared Surveyor: Design Overview and Current Status
- A simulation code for the infrared whole sky survey with the Far-Infrared Surveyor(FIS) on board ASTRO-F
- Water Vapor in AGB Stars
- High-Resolution Spectroscopy of Evolved Stars: from ISO to HII/L2
- Department of SiC Mirror for ASTRO-F