| Project/Area Number |
06640350
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| Research Category |
Grant-in-Aid for General Scientific Research (C)
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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 |
NOGUSHI Kunio National Astronomical Observatory, Division of Optical and Infrared Astronomy, Associate Professor, 理学部, 助教授 (10111824)
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| Co-Investigator(Kenkyū-buntansha) |
SATO Shuji Nagoya Unibersity, School of Science, Professor, 理学部, 教授 (50025483)
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| Project Period (FY) |
1994 – 1995
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| Project Status |
Completed (Fiscal Year 1995)
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| Budget Amount *help |
¥2,200,000 (Direct Cost: ¥2,200,000)
Fiscal Year 1995: ¥900,000 (Direct Cost: ¥900,000)
Fiscal Year 1994: ¥1,300,000 (Direct Cost: ¥1,300,000)
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| Keywords | Observations of Infrared spectra / Evolution of AGB stars / Circumstellar dust |
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| Research Abstract |
The scientific objective of this project is to clarify the evolution of asymptotic giant branch (AGB) stars by investigating the relation between evolutionary stages and the structure of circumstellar dust envelopes (CDE). At the beginning of this project, we consicered that it is very important to trace the evolutionary change of the structure of CDE observationally. Thus we observed variety of AGB stars with CDE in the near-infrared (NIR) wavelength region. As this observational results, we found that the space distribution of carbon stars (one kind of AGB stars) is likely to be different from that of O-rich AGB stars with thickCDE.This result indicate that the evolutionary process of AGB stars may depend on the location in the Galaxy caused by some difference in the physical condition which depends on the location. Thus we have newly observed about 450 carbon stars in the Galaxy in the NIR to clarify the difference in the space distribution of carbon stars from that of O-rich AGB stars. Our observed results suggest that the space distribution of carbon stars is different from that of O-rich AGB stars and that the evolutionary process of AGB stars depend on the location in the Galaxy.
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