| Project/Area Number |
06402004
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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 | The Institute of Space and Astronautical Science (ISAS) |
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Principal Investigator |
OKUDA Haruyuki The Institute of Space and Astronautical Science (ISAS) Div. Space Astrophysics Professor, 宇宙圏研究系, 教授 (50025293)
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| Co-Investigator(Kenkyū-buntansha) |
HIROMOTO Norihisa Communications Research Lab.Division Chief, 光技術部, 室長
SHIBAI Hiroshi Dept.Physics, Nagoya Univ.Professor, 大学院理学研究科, 教授 (70154234)
MURAKAMI Hiroshi The Institute of Space and Astronautical Science (ISAS) Div.Space Astrophysics P, 宇宙圏研究系, 教授 (40135299)
YAMAGAMI Takamasa The Institute of Space and Astronautical Science (ISAS) Div.Space Systems Eng.As, システム研究系, 助教授 (40013718)
YAJIMA Nobuyuki The Institute of Space and Astronautical Science (ISAS) Div.Space Systems Eng.Pr, システム研究系, 教授 (30200489)
中川 貴雄 宇宙科学研究所, 次世代探査機研究センター, 助教授 (20202210)
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| Project Period (FY) |
1994 – 1996
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| Project Status |
Completed (Fiscal Year 1996)
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| Budget Amount *help |
¥32,200,000 (Direct Cost: ¥32,200,000)
Fiscal Year 1996: ¥6,400,000 (Direct Cost: ¥6,400,000)
Fiscal Year 1995: ¥14,800,000 (Direct Cost: ¥14,800,000)
Fiscal Year 1994: ¥11,000,000 (Direct Cost: ¥11,000,000)
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| Keywords | Infrared Radiation / The Galaxy / Interstellar Matter / Interstellar Gas / Balloon-Borne Telescope / Far-Infrared Radiation / Spectroscopy / Star Fromation / 気球観測 |
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| Research Abstract |
It has widely been demonstrated that there exist various stages of gas, such as atoms, ions, and molecules in the interstellar space of the Galaxy. Among them, hydrogen 21 cm line and CO 2.6 mm line have been playing important roles in investigations of the galactic structure and physical and chemical stage of the Galaxy through the neutral hydrogen atomic gas and molecular gas, respectively. However, the previous result of our study by a [CII] far-Infrared line survey showed that there exists a new interstellar gas phase, "diffuse photodissociation region" . Photodissociation regions in the enterface region between the CO molecular gas and the hydrogen atomic gas, and are the dominant coolant by conversion of UV and optical radiation from luminous stars into the far-infrared radiation.
Therefore, the far-Infrared spectral lines are key for understanding the galactic interstellar space/matter, and are a tool for measuring the interstellar heavy element abundance. We have carried out a wide sky survey of [CII] 158 micron by a space infrared telescope ( IRTS ) and by a balloon-borne telescope ( BICE ), and [OI] 63 micron, [OIII] 52,88 micron, [CII] 158 micron, [NII] 122 micron, and [NIII] 57 micron lines by a European Infrared space observatory ( ISO ). From these data, we have shown diffuse photodissociation regions and diffuse ionization regions are important gas phases in the Galactic Interstellar space.
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