CHEMICAL INHOMOGENEITIES AMONG GIANT STARS IN NGC 3201

MUN-SUK CHUN

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CHEMICAL INHOMOGENEITIES AMONG GIANT STARS IN NGC 3201 KCI 등재 SCOPUS

MUN-SUK CHUN

언어ENG
URLhttps://db.koreascholar.com/Article/Detail/397700

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천문학회지 (Journal of The Korean Astronomical Society)

제21권 제1호 (1988.06)
pp.67-77

한국천문학회 (Korean Astronomical Society)

초록

Nine giant star's spectra in NGC 3201 were obtained using the image tube in Sutherland. From the analysis of these spectra we found the increase of Ca I and CH abundances with decreasing the radial distnace, but CN, Ca II and Fe abundances do not show this. Dependence of the calculated parameters seems to exist among CN, Ca I, Ca II and CH abundances.

ABSTRACT
I. INTRODUCTION
II. OBSERVATION
III. REDUCTION
IV. DISCUSSIONS
V. CONCLUSION
REFERENCES

저자

MUN-SUK CHUN(Department of Astronomy & Meteorology, Yonsei University)

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