Combining the AKARI Point Source Catalog and the 37-month Monitor of All-sky X-ray Image (MAXI) catalog, the infrared and X-ray properties of nearby active galactic nuclei were investigated. The 37-month MAXI catalog tabulates 100 nearby Seyfert galaxies, 73 of which are categorized into Seyfert I galaxies. Among these Seyfert galaxies, 69 ones were found to have an AKARI infrared counterpart. For the Seyfert I galaxies in this sample, a well-known correlation was found between the infrared and X-ray luminosities. However, the observed X-ray luminosity of the Seyfert II galaxies tends to be lower for the infrared luminosity than the Seyfert I galaxies. This suggests that the X-ray absorption is significant in the Seyfert II galaxies. The Seyfert II galaxies seem to have a bimodal distribution of the IR color between 18 μm and 90 μm. Especially, a large fraction of the Seyfert II galaxies exhibits a redder IR color than the Seyfert I galaxies. A possible origin of the redder IR color is brie y discussed, in relation to the star formation activity in the host galaxy, and to the X-ray absorption.

Recognition of the role of radio galaxies in the universe has been increasing in recent years. Their colossal energy output over huge volumes is now widely believed to play a key role not only in the formation of galaxies and their supermassive black holes, but also in the evolution of clusters of galaxies and, possibly, the cosmic web itself. In this regard, we need to understand the in ation of radio bubbles in the hot gas atmospheres of clusters and the importance of the role that radio galaxies play in the overall energy budget of the intracluster medium. Here, we present results from X-ray and radio band observations of the hot gas atmospheres of powerful, nearby radio galaxies in poor clusters.

We present an analysis of the soft X-ray emission of MRK 841 to investigate its long-term variation. The light variation of MRK 841 for three different energy bands of soft, medium, and hard values were studied. The maximum variability with a factor of 5 for about two years was confirmed at all three different bands. The light curves exhibit a gradual variation of brightness. In addition to a gradual variation, the short- term or micro variation was also confirmed with a factor of about two for all three different bands. The light variation of each band did not exhibit a correlation between them, but the flare event is strongest in the soft band. The hardness ratio for hard and soft bands shows irregular variation but there was no correlation between them. It was confirmed that there is a gradual decrease of the photon index. Results of our analysis are discussed within the framework of the accretion disk phenomenon.

본 논문에서는 고에너지 엑스선(6MeV)을 조사한 세포막 모델에서 K+-Na+ pump 시스템의 능동적 전달특성에 대하여 연구하였다. 이 실험에 사용된 세포막 모델은 Na+슬폰화 폴리스티렌-디비닐벤젠(polystyrene-divinylbenzene) 혼성 중합막을 사용하였다. 이온의 초기플럭스는 H+이온 농도의 증가와 함께 증가하였다. 이 실험의 조건을 pH 1.5-5, 온도 36.5℃로 하여 첫 번째, 방사선이 조사되지 않은 막에서 K+의 초기플럭스는 2.09x10-4-1.32x10-3mole/cm2·h이고 Na+의 초기플럭스는 7.09 x10-4-1.09x10-3mole/cm2·h으로 나타내었다. 두 번째, 방사선이 조사된 막에서 K+의 초기플럭스는 21.0x10-4-16.7x10-3mole/cm2·h이고 Na+의 초기플럭스는 62.0x10-4-20.6x10-3mole/cm2·h으로 나타내었다. 막의 K+/Na+선택도는 약 1.10이다. 조사된 막의 pH의 추진력은 조사되지 않은 막보다 약 9-20배 정도 유의성 있게 증가하였다. 세포막모델에서 K+-Na+의 pump 시스템의 능동적 전달특성이 비정상적이기 때문에 세포장해가 세포에서 발현된다고 사료된다.