본 연구는 보건계열 대학생을 대상으로 학습동기조절전략의 유형을 분 류하고, 이러한 유형에 따른 대학생 성공 및 삶의 만족도의 차이를 분석 하고자 하였다. G시 소재 대학 보건계열 학과(간호학과, 응급구조학과, 치위생학과)에 재학 중인 대학생 250명을 대상으로 한국형 학습동기조절 전략 척도, 대학생 성공 척도, 삶의 만족도 척도를 사용하여 자료를 수집 하였다. 수집된 자료는 군집분석, 다변량분산분석, 일원분산분석 등을 통 해 분석되었다. 연구 결과, 학습동기조절전략에 따라 '소극적 조절집단 (25.6%)', '중간 조절집단(39.6%)', '적극적 조절집단(34.8%)'의 세 가지 유형으로 분류되었다. 적극적 조절집단은 모든 전략에서 높은 점수를 보 였으며, 특히 사회적 인정/외적 보상 추구, 부모(교사)기대에 대한 보답, 공부에 대한 의무 등의 자기조절 전략에서 두드러진 활용 수준을 보였 다. 이러한 학습동기조절전략의 유형에 따라 대학생 성공의 모든 하위요 인과 삶의 만족도에서 유의미한 차이가 나타났다. 이러한 결과는 보건계 열 대학생의 학습동기조절전략이 학업적 성취를 넘어 대학생활의 다양한 측면에서의 성공과 전반적인 삶의 만족도와 밀접한 관련이 있음을 시사 한다.

In this paper, the formation and characterization of Pt2, Pt3 as well as Pt4 atomic clusters in cup-stacked carbon nanotubes (CSCNTs) are evaluated by DFT to examine the adsorption capacity under the clusters. The results show that the Pt clusters move toward the bottom edge or form rings in the optimized stable structure. Pt far from the carbon substrate possesses more active electrons and adsorption advantages. The three clusters can adsorb up to 17, 18, and 16 hydrogen molecules. Loading metal clusters at the bottom edge maintains a relatively good adsorption property despite the low binding energy through comparative studies. The adsorption capacity does not increase with the number of Pt for metal aggregation reducing the hydrogen adsorption area thus impacting the hydrogen storage ability and the aggregation phenomenon limiting the action of Pt metal. During adsorption, chemisorption occurs only in the Pt2 cluster, while multiple hydrogen molecules achieve physiochemical adsorption in the Pt3 and Pt4 clusters. Compared with the atomic loading of the dispersion system in equal quantities, the dispersion system features higher molecular stability and can significantly reduce the energy of the carbon substrates, providing more sites for hydrogen adsorption in space.

We investigate the evolution of initial fractal clusters at 3 kpc from the Galactic Center (GC) of the MilkyWay and show how red supergiant clusters (RSGCs)-like objects, which are considered to be the result of active star formation in the Scutum complex, can form by 16 Myr. We find that initial tidal filling and tidal over-filling fractals are shredded by the tidal force, but some substructures can survive as individual subclusters, especially when the initial virial ratio is ≤0.5. These surviving subclusters are weakly mass segregated and show a top-heavy mass function. This implies the possibility that a single substructured star cluster can evolve into multiple ‘star clusters’.

In this paper, we investigate asteroseismic scaling-relations of evolved stars in star clusters observed by Kepler/K2, aiming to address the issue of whether observed stellar oscillations are influenced by environmental factors, as there are interesting phenomena relating to the stellar pulsations observed in star clusters. Specifically, we compare statistical properties of distributions including Δν, νmax, HGauss, δνenv, and δν02 derived from red giant branch (RGB) and red clump (RC) stars in two pairs of star clusters: NGC 2682 - NGC 6819 and NGC 1817 - NGC 6811. We have found that the slopes of relations between νmax and Δν and between HGauss and νmax associated with RC stars in the more compact star clusters, NGC 2682 and NGC 1817, are in common less steep compared with those for NGC 6819 and NGC 6811. It is also found that the slopes of the relation between δνenv and νmax from RC stars in the more compact star clusters are in common steeper compared with those for the others. For the relation between δν02 and Δν obtained from RGB stars, the slope resulting from NGC 2682 and NGC 6819 is indistinguishable. The Kolmogorov–Smirnov tests conducted on RC stars in the pairs of NGC 2682 and NGC 6819, as well as NGC 1817 and NGC 6811, indicate that all the seismic quantities considered in this paper are drawn from different distributions. We conclude, therefore, that the properties of star clusters should be considered when asteroseismic data obtained from stars within star clusters are interpreted.