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논문 기본 정보

자료유형
학술저널
저자정보
Alexander Yushchenko (Astrocamp Contents Research Institute) Seunghyun Kim (Astrocamp Contents Research Institute Goyang) Yeuncheol Jeong (Sejong University) Aizat Demessinova (Al Farabi Kazakh National University) Volodymyr Yushchenko (Odessa National University) Dmytry Doikov (Odessa National Maritime University) Vira Gopka (Odessa National University) Kyung Sook Jeong (Sejong University) Pakakaew Rittipruk (National Astronomical Research Institute of Thailand)
저널정보
한국우주과학회 Journal of Astronomy and Space Sciences Journal of Astronomy and Space Sciences 제38권 제3호
발행연도
2021.9
수록면
175 - 183 (9page)

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The dependencies of the chemical element abundances in stellar atmospheres with respect to solar abundances on the second ionization potentials of the same elements were investigated using the published stellar abundance patterns for 1,149 G and K giants in the Local Region of the Galaxy. The correlations between the relative abundances of chemical elements and their second ionization potentials were calculated for groups of stars with effective temperatures between 3,764 and 7,725 K. Correlations were identified for chemical elements with second ionization potentials of 12.5 eV to 20 eV and for elements with second ionization potentials higher than 20 eV. For the first group of elements, the correlation coefficients were positive for stars with effective temperatures lower than 5,300 K and negative for stars with effective temperatures from 5,300 K to 7,725 K. The results of this study and the comparison with earlier results for hotter stars confirm the variations in these correlations with the effective temperature. A possible explanation for the observed effects is the accretion of hydrogen and helium atoms from the interstellar medium.

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