We have investigated the properties of thin film transistors(TFT) fabricated using zinc tin oxide(ZTO) thin films deposited via on-axis sputtering and FTS methods. ZTO thin films deposited by FTS showed lower root-mean-square(RMS) roughness and more uniformity than those deposited via on-axis sputtering. We observed enhanced electrical properties of ZTO TFT deposited via FTS. The ZTO films were deposited at room temperature via on-axis sputtering and FTS. The as-deposited ZTO films were annealed at 400 oC. The TFT using the ZTO films deposited via FTS process exhibited a high mobility of 12.91 cm2/V.s, a low swing of 0.80 V/decade, Vth of 5.78 V, and a high Ion/off ratio of 2.52 × 106.

We present the results of far-infrared spectral mapping of the Galactic center region with FIS-FTS, which covered the two massive star-forming clusters, Arches and Quintuplet. We find that two dust components with temperatures of about 20 K and 50 K are required to fit the overall continuum spectra. The warm dust emission is spatially correlated with the [OIII] 88 μm emission and both are likely to be associated with the two clusters, while the cool dust emission is more widely distributed without any clear spatial correlation with the clusters. We find differences in the properties of the ISM around the two clusters, suggesting that the star-forming activity of the Arches cluster is at an earlier stage than that of the Quintuplet cluster.

We present the results of far-infrared spectroscopic observations of the Large Magellanic Cloud (LMC) with FIS-FTS. We covered a large area across the LMC, including 30 Doradus (30 Dor) and N44 star-forming regions, by 191 pointings in total. As a result, we detect the [OIII] and [CII] line emission as well as far-infrared dust continuum emission throughout the LMC. We find that the [OIII] emission is widely distributed around 30 Dor. The observed size of the distribution is too large to be explained by massive stars in 30 Dor, which are assumed to be enshrouded by clouds with the constant gas density estimated from the [OIII] line intensities. Therefore the surrounding structure is likely to be highly clumpy. We also find a global correlation between the [OIII] and the far-infrared continuum emission, suggesting that the gas and dust are well mixed in the highly-ionized region where the dust survives in clumpy dense clouds shielded from energetic photons. Furthermore we find that the ratios of [CII]/CO are as high as 110,000 in 30 Dor, and 45,000 even on average, while they are typically 6,000 for star-forming regions in our Galaxy. The unusually high [CII]/CO is also consistent with the picture of clumpy small dense clouds.

Diese Arbeit ist gegen das Urteil vom Obersten Gericht(2005.4.15, 2004do8701) ausgebildet. Es geht hier um die Frage, welche Voraussetzungen notwendig sind, damit die dem wesentlichen Geschäft begleitende Geschäftssache unter dem Tatbestand des Geschäftshindernis subsumiert werden kann, besonders ob die einmalige Geschäftssache ebenso wie der Umzug der Fabrik in der Gesellschaft zum 'Geschäft' gehört, das im Strafrecht §314-Ⅰ bestimmt ist. Nach meiner Analysierung ist das Oberste Gericht der Auffassung, dáß die dem Hauptgeschäft begleitende einmalige Geschäftssache zum sogenannten 'Geschäft' gehört werden kann, wenn dieselbe zwei Bedingungen, erstens die enge Beziehung mit dem Hauptgeschäft und zweitens die Dauerhaftigkeit erfüllt. Es ist aber meiner Meinung, dáß solche Stellung des Obersten Gerichts problematisch in mancher Weise ist, und deshalb unannehmbar ist.