| Project/Area Number |
58420004
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| Research Category |
Grant-in-Aid for General Scientific Research (A)
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| Allocation Type | Single-year Grants |
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| Research Field |
Astronomy
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| Research Institution | Nagoya University |
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Principal Investigator |
KAWABATA Kin-aKi Department of Astrophysics, Nagoya University, Professor, 理学部, 教授 (60022513)
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| Co-Investigator(Kenkyū-buntansha) |
TAKANO Toshiaki J.S.P.S., Post Doctoral Fellow, 特別研究員
OGAWA Hideo Department of Astrophysics, Nagoya University, Reseach Associate, 理学部, 助手 (20022717)
FUKUI Yasuo Department of Astrophysics, Nagoya University, Associate Professor, 理学部, 助教授 (30135298)
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| Project Period (FY) |
1983 – 1985
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| Project Status |
Completed (Fiscal Year 1988)
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| Budget Amount *help |
¥34,700,000 (Direct Cost: ¥34,700,000)
Fiscal Year 1985: ¥2,000,000 (Direct Cost: ¥2,000,000)
Fiscal Year 1984: ¥2,000,000 (Direct Cost: ¥2,000,000)
Fiscal Year 1983: ¥30,700,000 (Direct Cost: ¥30,700,000)
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| Keywords | interstellar molecules / star formation / radio astronomy / ミリ波望遠鏡 |
|---|
| Research Abstract |
We found 14 separate ^<13>CO features with different radial velocities and locations toward the Orion Nebula. It is shown that these features are in dyanmically stable equillibrium and the mass of the features are small. It is suggested that HII expansion is not effective in triggering formation of massive stars, and that newly formed stars are less massive even if stars are formed.
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