| Project/Area Number |
11304011
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| Research Category |
Grant-in-Aid for Scientific Research (A)
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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 | Nagoya University |
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Principal Investigator |
SHIBAI Hiroshi Nagoya University, Graduate School of Science, Professor, 大学院・理学研究科, 教授 (70154234)
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| Co-Investigator(Kenkyū-buntansha) |
NAKAGAWA Takao Inst. Sp. Astronaut. Sci., Professor, 宇宙圏研究系, 教授 (20202210)
SATO Shinji Nagoya University, Graduate School of Science, Res. Assoc., 大学院・理学研究科, 助手 (60192598)
KAWADA Mitsunobu Nagoya University, Graduate School of Science, Lecturer, 大学院・理学研究科, 講師 (50280558)
DOI Yasuo University of Tokyo, Res. Assoc., 大学院・総合文化研究科, 助手 (70292844)
藤原 幹生 郵政省通信総合研究所, 光技術部, 主任研究官
廣本 宣久 郵政省, 通信総合研究所・企画部, 主任研究官
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| Project Period (FY) |
1999 – 2001
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| Project Status |
Completed (Fiscal Year 2001)
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| Budget Amount *help |
¥37,860,000 (Direct Cost: ¥34,800,000、Indirect Cost: ¥3,060,000)
Fiscal Year 2001: ¥13,260,000 (Direct Cost: ¥10,200,000、Indirect Cost: ¥3,060,000)
Fiscal Year 2000: ¥10,200,000 (Direct Cost: ¥10,200,000)
Fiscal Year 1999: ¥14,400,000 (Direct Cost: ¥14,400,000)
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| Keywords | Infrared Radiation / Galaxies / Interstellar Medium / Interstellar Gas / Far-Infrared Radiation / Balloon-Borne Telescope / Star Formation / Infrared Sensor |
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| Research Abstract |
The purpose of this research is to diagnose interstellar gas in nearby galaxies and to understand the ionization/dissociation structure of the interstellar space of the Galaxy as well as the energy transfer flow there by line spectroscopy in the far-infrared region.
At first, we have developed a new type reflection grating, 'immersion grating1, which is relatively small although it has higher spectral resolution. By using silicon whose refractive index is 3.4, the spectral resolving power of 10,000 is achieved with a 10 cm grating. The anti-reflection coating is also technically feasible. We have measured the transmission of a large silicon material that is to be actually used for the grating at a cryogenic temperature (4K) by developing a new device that is necessary for this kind of measurement, and the result is more than 50 %. Moreover, we designed a two-dimensional array as well as a cryogenic optical system for the spectrometer.
In parallel to this, by analyzing the data taken by the ISO (ESA) satellite, we have an important knowledge about the silicon abundance in the interstellar space of the Carina region, a typical large-scale star-forming region. We also found a new method to estimate the physical characteristics of the interstellar dust grain from a fewer observational data in the far-infrared region. These result were submitted to main journals.
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