| Project/Area Number |
11304010
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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 University of Tokyo |
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Principal Investigator |
YAMAMOTO Satoshi The University of Tokyo, Graduate School of Science, Professor, 大学院・理学系研究科, 教授 (80182624)
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| Co-Investigator(Kenkyū-buntansha) |
NOGUCHI Takashi National Astronomy Observatory, Division of Radio Astronomy, Associate Professor, 電波天文学研究系, 助教授 (90237826)
SEKIMOTO Yutaro National Astronomy Observatory, Division of Radio Astronomy, Associate Professor, 電波天文学研究系, 助教授 (70262152)
OKA Tomoharu The University of Tokyo, Graduate School of Science, Assistant, 大学院・理学系研究科, 助手 (10291056)
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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 |
¥33,960,000 (Direct Cost: ¥33,000,000、Indirect Cost: ¥960,000)
Fiscal Year 2001: ¥4,160,000 (Direct Cost: ¥3,200,000、Indirect Cost: ¥960,000)
Fiscal Year 2000: ¥14,100,000 (Direct Cost: ¥14,100,000)
Fiscal Year 1999: ¥15,700,000 (Direct Cost: ¥15,700,000)
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| Keywords | terahertz-wave / Submillimeter-wave / molecular cloud / Galaxy / radio telescope / neutral carbon atom / superconductivity / 電波天文学 / 中世炭素原子 / 星間化学 |
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| Research Abstract |
In the present study, we have developed the sensitive receiver system installed on the Mount Fuji submillimeter-wave telescope in order to conduct the large-scale mapping observations of the neutral carbon atom. We achieved the DSB noise temperature of 120 K at 492 GHz and 580 K at 809 GHz. These are the top class performance among the submillimeter-wave receivers continuously used in the astronomical observations.
With this sensitive receiver, we have conducted large-scale mapping observation of the 492 GHz line of the neutral carbon atom toward many nearby molecular clouds including Orion A giant molecular cloud and Taurus dark cloud complex. Furthermore, we have mapped several representative star-forming regions with the 809 GHz line of the neutral carbon atom for the first time. From these results, we found that the abundance of the neutral carbon atom is not strongly dependent on the UV field strength, but on the evolutionary stage of molecular clouds.
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