Journal of The Korean Astronomical Society (천문학회지)
- Volume 24 Issue 1
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- Pages.25-53
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- 1991
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- 1225-4614(pISSN)
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- 2288-890X(eISSN)
THE EVOLUTION OF A SPIRAL GALAXY: THE GALAXY
- Lee, See-Woo (Department of Astronomy, Seoul National University) ;
- Park, Byeong-Gon (Department of Astronomy, Seoul National University) ;
- Kang, Yong-Hee (Department of Earth Science Education, Kyungpook National University) ;
- Ann, Hong-Bae (Department of Earth Science Education, Pusan National University)
- Published : 1991.06.30
Abstract
The evolution of the Galaxy is examined by the halo-disk model, using the time-dependent bimodal IMF and contraints such as cumulative metallicity distribution, differential metallicity distribution and PDMF of main sequence stars. The time scale of the Galactic halo formation is about 3Gyr during which the most of halo stars and metal abundance are formed and
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