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Numerical simulation of the crack propagation behavior in 3D elastic body
Taniguchi, Takeo,Miyaji, Akihiko,Suetsugu, Takeshi,Matsunaga, Shohgo Techno-Press 1994 Structural Engineering and Mechanics, An Int'l Jou Vol.2 No.3
The purpose of this investigation is to propose a numerical simulation method of the crack propagation behavior in 3-dimensionl elastic body. The simulation method is based on the displacement-type finite element method, and the linear fracture theory is introduced. The results from the proposed method are compared with those from the structural experiments, and the good coincidences between them are shown in this paper. At the same time, 2-dimensional analysis is also done, and the results are compared with those obtained from 3-dimensional analysis and the structural experiments.
ERRATUM : 'LYMANα EMITTERS BEYOND REDSHIFT 5: THE DAWN OF GALAXY FORMATION' (JKAS, 36, 123, [2003])
Taniguchi, Yoshiaki,Shioya, Yasuhiro,Ajiki, Masaru,Fujita, Shinobu S.,Nagao, Tohru,Murayama, Takashi The Korean Astronomical Society 2003 Journal of The Korean Astronomical Society Vol.36 No.4
The first sentence in the second paragraph of INTRODUCTION, 'The first discovery of a galaxy beyond z=5 was reported by Weymann et al. (1998); HDF 4-470.3 at z=5.60.' should be read as 'The first discovery of a galaxy beyond z=5 was reported by Dey et al. (1998); 0140+326 RD1 at z=5.34'. The authors sincerely regret this error.
Taniguchi, Shin-Ichi,Shong, Minho,Giuliani, Cesidio,Napolitano, Giorgio,Saji, Motoyasu,Montani, Valeria,Suzuki, Koichi,Singer, Dinah S.,Kohn, Leonard D. 충남대학교 생물공학연구소 1999 생물공학연구지 Vol.7 No.-
Increased MHC class I expression on thyrodytes is evident in ATD (4, 21) and has been suggested to be an important causal factor in the development or perpetuation of disease expression (3). The hypothesis has been offered that the elevations result in abnormal presentation of thyroid antigens to immune cells, thereby breaking tolerance, and that this elicits the clonal expansion of autoreactive T cells associated with disease expression (3).
THE HST COSMOS PROJECT: CONTRIBUTION FROM THE SUBARU TELESCOPE
TANIGUCHI YOSHIAKI,SCOVILLE N. Z.,SANDERS D. B.,MOBASHER B.,AUSSEL H.,CAPAK P.,AJIKI M.,MURAYAMA T.,MIYAZAK S.,KOMIYAMA Y.,SHIOYA Y.,NAGAO T. The Korean Astronomical Society 2005 Journal of The Korean Astronomical Society Vol.38 No.2
The Cosmic Evolution Survey (COSMOS) is a Hubble Space Telescope (HST) treasury project. The COSMOS aims to perform a 2 square degree imaging survey of an equatorial field in I(F814W) band, using the Advanced Camera for Surveys (ACS). Such a wide field survey, combined with ground-based photometric and spectroscopic data, is essential to understand the interplay between large scale structure, evolution and formation of galaxies and dark matter. In 2004, we have obtained high-quality, broad band images of the COSMOS field (B, V, r', i', and z') using Suprime-Cam on the Subaru Telescope, and we have started our new optical multi-band program, COSMOS-21 in 2005. Here, we present a brief summary of the current status of the COSMOS project together with contributions from the Subaru Telescope. Our future Subaru program, COSMOS-21, is also discussed briefly.
LYMANα EMITTERS BEYOND REDSHIFT 5: THE DAWN OF GALAXY FORMATION
TANIGUCHI YOSHIAKI,SHIOYA YASUHIRO,AJIKI MASARU,FUJITA SHINOBU S.,NAGAO TOHRU,MURAYAMA TAKASHI The Korean Astronomical Society 2003 Journal of The Korean Astronomical Society Vol.36 No.3
The 8m class telescopes in the ground-based optical astronomy together with help from the ultra-sharp eye of the Hubble Space Telescope have enabled us to observe forming galaxies beyond red shift z = 5. In particular, more than twenty Ly$\alpha$-emitting galaxies have already been found at z > 5. These findings provide us with useful hints to investigate how galaxies formed and then evolved in the early universe. Further, detailed analysis of Ly$\alpha$ emission line profiles are useful in exploring the nature of the intergalactic medium because the trailing edge of cosmic reionization could be close to z $\~$ 6 -7, at which forming galaxies have been found recently. We also discuss the importance of superwinds from forming galaxies at high redshift, which has an intimate relationship between galaxies and the intergalactic medium. We then give a review of early cosmic star formation history based on recent progress in searching for Ly$\alpha$-emitting young galaxies beyond red shift 5.