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Dietary Carob Pods on Growth Performance and Meat Quality of Fattening Pigs
Kotrotsios, Nikolaos,Christaki, Efterpi,Bonos, Eleftherios,Paneri, Panagiota Florou Asian Australasian Association of Animal Productio 2012 Animal Bioscience Vol.25 No.6
In this experiment the effect of dietary carob pods in the growth performance of fattening pigs and their meat quality, including steak chemical composition and fatty acid profile, were examined. A total of 160 weaning piglets, 30 days old, were allocated into four equal groups with 4 subgroups of 5 female and 5 males each. The animals were fed with isocaloric and isonitrogenous diets, containing either 0 or 75 or 100 or 125 g of carob pods per kg of feed. At the end of the experiment, on the 180 day of age, carcass subcutaneous fat thickness, steak chemical composition and steak fatty acid profile were determined. The results of the experiment showed that the dietary addition of 75 or 100 g/kg carob pods increased body weight at slaughter and carcass weight. No significant effect was noticed on the other examined carcass parameters. Consequently, carob pods could be suggested as a potential feed for fattening pigs without any adverse effect on their meat quality.
Talents First!: Wu Ta-you and Science Policy Infrastructures in the Republic of China (1927-1970)
( Chang Kuo-hui ),( Gary Lee Downey ),( Shih Bono Po-jen ) 한국과학사학회 2020 한국과학사학회지 Vol.42 No.2
A main theme in the history of science policy in Taiwan concerns the positioning of science infrastructures in nation building and rapid economic growth. This article calls attention to another evolving initiative in science policy in the Republic of China (ROC), one that emphasized the production of talents who could become societal leaders, including by working for and within government. We trace the emergence of this initiative through the career of Wu Ta-you, who grew up in mainland China, earned his Ph.D. in the United States, and worked on the margins of reconstruction during the 1930s. Through the 1950s, he played a leadership role advocating for long-term planning to develop fundamental researchers in science in Taiwan. His moment appeared to come in 1967 when he became the president’s chief science adviser. His efforts to develop science talents were soon displaced, however, by emerging shorter-term initiatives to support the military and industry. Clearly not contributing as an instrumental technocrat nor a proponent for autonomous basic research, was he attempting to combine the identity of a scientist with that of the Chinese scholar-official? By taking science policy in a different direction, the ROC, in Wu’s terms, remained stuck on the surface of science.
Lee, Myung Gyoon,Jang, In Sung,Beaton, Rachael,Seibert, Mark,Bono, Giuseppe,Madore, Barry American Astronomical Society 2017 ASTROPHYSICAL JOURNAL LETTERS - Vol.835 No.2
<P>Ultra-faint dwarf galaxies (UFDs) are the faintest known galaxies, and due to their incredibly low surface brightness, it is difficult to find them beyond the Local Group. We report a serendipitous discovery of a UFD, Fornax UFD1, in the outskirts of NGC 1316, a giant galaxy in the Fornax cluster. The new galaxy is located at a projected radius of 55 kpc in the south-east of NGC 1316. This UFD is found as a small group of resolved stars in the Hubble Space Telescope images of a halo field of NGC 1316, obtained as part of the Carnegie-Chicago Hubble Program. Resolved stars in this galaxy are consistent with being mostly metal-poor red giant branch (RGB) stars. Applying the tip of the RGB method to the mean magnitude of the two brightest RGB stars, we estimate the distance to this galaxy, 19.0. +/-. 1.3 Mpc. Fornax UFD1 is probably a member of the Fornax cluster. The color-magnitude diagram of these stars is matched by a 12 Gyr isochrone with low metallicity ([Fe/H]approximate to-2.4). Total magnitude and effective radius of Fornax UFD1 are M-V approximate to -7.6 +/- 0.2 mag and r(eff) = 146 +/- 9 pc, which are similar to those of Virgo UFD1 that was discovered recently in the intracluster field of Virgo by Jang & Lee. Fornax UFD1 is the most distant known UFD that is confirmed by resolved stars. This indicates that UFDs are ubiquitous and that more UFDs remain to be discovered in the Fornax cluster.</P>
Topology optimization of bracing systems in buildings considering the effects of the wind
Paulo U. Silva,Rayanne E.L. Pereira,Gustavo Bono 국제구조공학회 2023 Structural Engineering and Mechanics, An Int'l Jou Vol.86 No.4
Nowadays, urban centers are increasingly vertical, making architects and engineers look for more efficient tools to analyze the effects of wind on tall buildings. Topology optimization can be used as an efficient tool for the design of bracing systems. Therefore, this work obtained the wind loads that act in the CAARC building, following the Brazilian standard NBR 6123/1988 and using Computational Fluid Dynamics. Four loading situations were considered, using the SIMP and BESO methods to optimize two-dimensional structures. A comparison between the SIMP and BESO methods is presented, showing the differences in the geometry of the solution found by both methods, the percentage variation in the objective function values and the dimensionless processing time. The solutions obtained through the loads obtained by the Brazilian standard are also compared with the numerical solutions obtained by CFD. The results show that the BESO method presented more rigid structures compared to the SIMP method. The bracing structures obtained with the SIMP method always present similar patterns in the distribution and quantity of bars, in contrast to the BESO method where no characteristic topology pattern was observed. It was concluded that even though the structures obtained by the BESO method presented greater stiffness, the SIMP method was less susceptible to the methodology used for the determination of wind loads. Additionally, it was evident the great potential that the combination topology optimization and computational wind engineering have in the design of bracing systems of high functional and aesthetic standards.
THE RR LYRAE VARIABLES AND HORIZONTAL BRANCH OF NGC 6656 (M22)<sup>,</sup>
Kunder, Andrea,Stetson, Peter B.,Cassisi, Santi,Layden, Andrew,Bono, Giuseppe,Catelan, Má,rcio,Walker, Alistair R.,Paredes Alvarez, Leonardo,Clem, James L.,Matsunaga, Noriyuki,Salaris, Maurizio American Institute of Physics 2013 The Astronomical journal Vol.146 No.5
<P>The first calibrated broadband UBVI time-series photometry is presented for the RR Lyrae variable stars in NGC 6656 (M22), with observations spanning a range of 22 years. We have also redetermined the variability types and periods for the RR Lyrae stars identified previously by photographic observations, revising the number of fundamental-mode RR Lyrae variables (RR0) to 10 and the number of first-overtone variables (RR1) to 16. The mean periods of the RR0 and RR1 variables are 〈P〉<SUB>RR0</SUB> = 0.66 ± 0.02 days and 〈P〉<SUB>RR1</SUB> = 0.33 ± 0.01 days, respectively, supporting an Oosterhoff II classification for the cluster. The number ratio of RR1-type to all RR-type variables is N<SUB>1</SUB>/N<SUB>RR</SUB> = 0.61, also consistent with an Oosterhoff II designation. Both the RR Lyrae stars' minimum light colors and the blue edge of the RR Lyrae instability strip suggest E( B – – V) = 0.36 ± 0.02 mag toward M22. Regarding the HB morphology of M22, we find (B-R)/(B+V+R) = +0.97 ± 0.1 and at least one 'gap' located in an unusual part of the blue HB, in the middle of the so-called hot HB stars.</P>
木庭康樹(Koki Kiniwa),大江淳悟(Jungo Ohe),房野?也(Shinya Bono),丸山啓史(Keishi Maruyama),磨井祥夫(Sachio Usui),沖原謙(Ken Okihara),伊藤?馬(Kzuma Ito),菅輝(Akira Kan),?川?久(Mitsuhisa Shiokawa) 한국체육과학회 2010 한국체육과학회지 Vol.19 No.1
The purpose of this study is to show objective data about the amount of the activity of the referee in an actual game, and to use these for the referee training in the future. As a result of consideration, the main referee became clear that an equal ability of moved distance, the movement speed, and the turn frequency, etc. with the field player was demanded. The main referee showed total moved distance twice the sub?referee, and this moved distance was almost equal to the field player. Moreover, it has been understood that a considerably high ability is demanded from the main referee about brilliant because the frequency about four times the sub?referee of the turn is done. Therefore, the main referee is doing advanced work of giving a decision while equal stamina's with the field player being demanded and repeating the turn and the movement according to a diagonal method. On the other hand, the moved distance of the sub?referee was main referee and field player's halves. Moreover, it is thought that the sub?referee is giving the judgment (offside and ball out) in the stopped state at the moment from low?speed movement frequency high. The future tasks are to analyze the accuracy of the work of the sub?referee by comparing sub?referee's position with the position of an offside line, and to consider the sub ?referee qualitatively.