| Project/Area Number |
11640237
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| Research Category |
Grant-in-Aid for Scientific Research (C)
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| Allocation Type | Single-year Grants |
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| Section | 一般 |
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| Research Field |
Astronomy
|
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| Research Institution | Osaka Kyoiku University |
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Principal Investigator |
SADAKANE Kozo Osaka Kyoiku Univ. Faculty of Education, Professor, 教育学部, 教授 (20110794)
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| Project Period (FY) |
1999 – 2002
|
| Project Status |
Completed (Fiscal Year 2002)
|
| Budget Amount *help |
¥3,500,000 (Direct Cost: ¥3,500,000)
Fiscal Year 2002: ¥700,000 (Direct Cost: ¥700,000)
Fiscal Year 2001: ¥600,000 (Direct Cost: ¥600,000)
Fiscal Year 2000: ¥600,000 (Direct Cost: ¥600,000)
Fiscal Year 1999: ¥1,600,000 (Direct Cost: ¥1,600,000)
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| Keywords | Staro / Spectroscopy / Chemical Composition / Galaxy / Chemical Evolution / 恒星分光 / 金属欠乏星 / 銀河の化学進化 / 天体スペクトル / すばる望遠鏡 / 恒星分光学 |
|---|
| Research Abstract |
Using the High Dispersion Spectrograph (HDS) on the SUBARU telescope, I obtained many scientic data during the commissioning phase of the spectrograph (2001, July 〜2002, March). Abundance analyses of more than 10 metal deficient halo stars have been carried out using high quality spectroscopic data obtained in 2001 and 2002, Kesulte will be published in papers within 2003.
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