• 제목/요약/키워드: JY

검색결과 175건 처리시간 0.027초

아말감과 이종(異種)금속의 거리에 따른 부식에 대한 고찰 (A Study on Corrosion according to Distance between Amalgam and Dissimilar Metals)

  • 김주원;정은경
    • 치위생과학회지
    • /
    • 제4권3호
    • /
    • pp.103-109
    • /
    • 2004
  • 본 실험은 제조회사 매뉴얼과 통법에 의해서 Amalgam 합금, Ni-Cr alloy의 Crown용 Verabond, Denture용 Talladium $^{TM}alloy$로 각각 24개의 총 72의 시편을 하악 제1대구치근 원심 치관 폭경과 임상에서의 MOD cavity를 고려하여 제작하였고 인공 타액 80ml를 담은 200ml 용 비이커에 시편을 넣어 0mm, 7mm, 40mm 거리에서 7일 후 갈바닉 부식을 측정하였다. 유리금속은 유도 플라즈마 방출 분광기(Inductively Coupled Plasma - Atomic Emission Spectrometer(ICP-AES, JY-50P, VG Elemental Co. France)로 전해액내의 Cu, Ag, Ni, Cr, Sn, Zn, Hg를 정량 분석했으며 그 결과 다음과 같은 결론을 얻었다. 첫째, Cu, Sn, Ag, Hg, Zn은 아말감이 금 합금과 접촉했을 때가 크라운용 Ni-Cr alloy와 덴쳐용 Talladium alloy 보다 아주 많이 유리 했으며 금 합금이 구강조직과 생체 적합성이 가장 좋다지만 아말감과 함께 있을 때 가장 불리 했슴을 알 수 있었다. 둘째, 아말감이 금 합금과 접촉했을 때, 금 합금의 조성에서 Ni, Cr 같은 중금속이 함유되지 않았기 때문인지 전혀 유리되지 않았으나 Sn은 조성에는 없었지만 $227.1{\pm}18.0035{\mu}g/cm^2$나 유리 되었고 Hg도 유리되었는데 이는 아말감 자체의 유리 물질임을 추측할 수 있었다. 셋째, 아말감 합금과 금 합금 사이에서의 0mm, 7mm, 40mm 거리에서는 Cu, Ag는 유의성이 있었으며 Hg는 유의성이 없었다. 이는 금합금은 절대 아말감과 같이 사용해서 안되며 이종 보철물 사이의 거리에 관계없이 사용을 금해야 하는 것으로 사료된다. 넷째, 아말감합금이 Crown용 Ni-Cr 합금과 접촉했을 때 아말감의 Ag이 유리 되지 않았으며 Zn, Ni, Sn, Hg, Cu의 순으로 유리되었다. 0mm, 7mm, 40mm 거리에 따라서 유의성이 있었다. Hg는 유리 되지 않았지만 중금속인 Ni, Cr은 유리되었고 반대 악궁이나 거리가 떨어져 있으면 접촉보다 Hg의 유리가 적었다. 다섯째, 아말감합금이 Denture용 Talladium alloy 합금과 접촉했을 때 0mm, 7mm, 40mm 거리에서도 유의성이 있었다. 0mm, 7mm, 40mm 거리에 따라서 유의성이 있었다. Hg는 유리 되지 않았지만 중금속인 Ni, Cr은 유리되었고 반대 악궁이나 거리가 떨어져 있으면 접촉보다 Hg의 유리가 적었다. 여섯째, 인공 타액에서 접촉 시 Amalgam alloy와 Gold, Verabond, Talladium alloy의 Cu, Sn, Ag, Hg, Zn, Ni, Cr의 ICPES 검사 결과 Cu, Hg가 유의성을 있었다. 일곱째, 인공타액에서 아말감합금과 두 비귀금속인 Ni-Cr alloy(crown용), Denture용 Talladium alloy가 접촉한 경우 거리에 따른 Hg, Ni, Cr의 유리 부산물에서 유의성을 확인했다.

  • PDF

No asymmetric outflows from Sagittarius A* during the pericenter passage of the gas cloud G2

  • Park, Jong-Ho;Trippe, Sascha;Krichbaum, Thomas;Kim, Jae-Young;Kino, Motoki;Bertarini, Alessandra;Bremer, Michael;de Vicente, Pablo
    • 천문학회보
    • /
    • 제40권1호
    • /
    • pp.73.2-74
    • /
    • 2015
  • The gas cloud G2 falling toward Sagittarius A* (Sgr A*), the supermassive black hole at the center of the Milky Way, is supposed to provide valuable information on the physics of accretion flows and the environment of the black hole. We observed Sgr A* with four European stations of the Global Millimeter Very Long Baseline Interferometry Array (GMVA) at 86 GHz on 1 October 2013 when parts of G2 had already passed the pericenter. We searched for possible transient asymmetric structure - such as jets or winds from hot accretion flows - around Sgr A* caused by accretion of material from G2. The interferometric closure phases (which are zero if the spatial brightness distribution of the target is symmetric, and deviate from zero otherwise) remained zero within errors during the observation time. We thus conclude that Sgr A* did not show significant asymmetric (in the observer frame) outflows in late 2013. Using simulations, we constrain the size of the outflows that we could have missed to ${\approx}2.5$ mas along the major axis, ${\approx}0.4$ mas along the minor axis of the beam, corresponding to approximately 232 and 35 Schwarzschild radii, respectively; we thus probe spatial scales on which the jets of radio galaxies are suspected to convert magnetic into kinetic energy. As probably less than 0.2 Jy of the flux from Sgr A* can be attributed to accretion from G2, one finds an effective accretion rate ${\eta}M{\leq}1.5{\times}10^9kg/s{\approx}7.7{\times}10^{-9}M_{earth}/yr$ for material from G2. Exploiting the kinetic jet power-accretion power relation of radio galaxies, one finds that the rate of accretion of matter that ends up in jets is limited to $M{\leq}10^{17}kg/s{\approx}0.5M_{Earth}/yr$ less than about 20% of the mass of G2. Accordingly, G2 appears to be largely stable against loss of angular momentum and subsequent (partial) accretion at least on time scales ${\leq}1$ year.

  • PDF

GALAXIES ON DIET: FEEDBACK SIGNATURES IN RADIO-AGN HOST GALAXIES

  • Karouzos, Marios;Im, Myungshin;Trichas, Markos;Goto, Tomogotsu;Malkan, Matthew;Ruiz, Angel;Jeon, Yiseul;Kim, Ji Hoon;Lee, Hyung Mok;Kim, Seong Jin;Oi, Nagisa;Matsuhara, Hideo;Takagi, Toshinobu;Murata, Kazumi;Wada, Takehiko;Wada, Kensuke;Shim, Hyunjin;Hanami, Hitoshi;Serjeant, Stephen;White, Glenn;Pearson, Chris;Ohyama, Youichi
    • 천문학논총
    • /
    • 제32권1호
    • /
    • pp.201-203
    • /
    • 2017
  • There exists strong evidence supporting the co-evolution of central supermassive black holes and their host galaxies; however it is still under debate how such a relation comes about and whether it is relevant for all or only a subset of galaxies. An important mechanism connecting AGN to their host galaxies is AGN feedback, potentially heating up or even expelling gas from galaxies. AGN feedback may hence be responsible for the eventual quenching of star formation and halting of galaxy growth. A rich multi-wavelength dataset ranging from the X-ray regime (Chandra), to far-IR (Herschel), and radio (WSRT) is available for the North Ecliptic Pole field, most notably surveyed by the AKARI infrared space telescope, covering a total area on the sky of 5.4 sq. degrees. We investigate the star formation properties and possible signatures of radio feedback mechanisms in the host galaxies of 237 radio sources below redshift z = 2 and at a radio 1.4 GHz flux density limit of 0.1 mJy. Using broadband SED modelling, the nuclear and host galaxy components of these sources are studied simultaneously as a function of their radio luminosity. Here we present results concerning the AGN content of the radio sources in this field, while also offering evidence showcasing a link between AGN activity and host galaxy star formation. In particular, we show results supporting a maintenance type of feedback from powerful radio-jets.

원심모형실험을 통한 차량방호울타리 지지말뚝의 수평방향 충격하중에 대한 극한지지력 (Ultimate Capacity of Guardrail Supporting Pile Subjected to Lateral Impact Load Using Centrifuge Model Test)

  • 윤종석;이민지;추연욱
    • 한국지반공학회논문집
    • /
    • 제35권11호
    • /
    • pp.25-36
    • /
    • 2019
  • 차량이 도로를 이탈하여 성토부로 추락하는 것을 방지하기 위해 설치되는 연성 차량방호울타리는 사면부 시작점 근처에 도로방향으로 일렬로 근입된 무리말뚝과 무리말뚝 위에 부착되는 가드레일로 구성되어 있다. 차량방호울타리에 차량 충돌 시, 충돌에너지의 일부는 가드레일의 변형에 의해 흡수되며, 나머지 에너지는 가드레일을 지지하는 말뚝과 지반의 상호작용으로 저항하게 된다. 본 논문에서는 충격하중에 대한 말뚝과 지반의 상호작용을 원심모형실험을 수행하여 분석하였다. 풍화토로 다져진 경사지반에 설치된 단말뚝의 충격하중에 대한 극한지지력 및 거동특성을 분석하고자 하였다. 이를 위해 말뚝에 충격하중을 모사할 수 있는 하중재하시스템을 설계 및 구축하였다. 구축된 원심모형실험체 및 하중재하시스템을 이용하여 하중 및 지반조건에 대한 매개변수연구를 수행하였다. 최종적으로, 말뚝의 하중재하점에서 나타나는 하중-변위 곡선을 계측하여 충격극한지지력을 분석하였다. 또한, 휨모멘트 분포도로부터 산정된 지반반력 분포도를 도출하였고, 선행 연구결과와 비교하여 차량 방호울타리 지지말뚝의 지지거동을 분석하였다.

Gadoxetic acid 조영증강 자기공명영상에서 숙임각 변화에 따른 국소 간종양 검출능 비교 (Improved Focal Liver Lesion Detection by Increasing Flip Angle During Gadoxetic Acid-Enhancement in MRI)

  • 이세지;김영근
    • 대한방사선기술학회지:방사선기술과학
    • /
    • 제38권2호
    • /
    • pp.115-120
    • /
    • 2015
  • Gadoxetic acid (GA) 조영증강 자기공명(MR) 영상에서 일반적으로 많이 이용되는 숙임각(flip angle, FA) $11^{\circ}$와 비교하여 FA $30^{\circ}$를 이용한 3분, 10분 및 15분 영상에서 국소성 간 병변 검출 차이를 알아보고자 하였다. 대상 및 방법 : 3.0T MR 기기로 GA 조영증강지연기 MR영상을 시행 받은 69명의 환자를 대상으로 하였다. 대상 환자는 간세포암 23명과 전이암 12명으로 총 35명(남성 23, 여성12, 평균연령 60.4세)이었다. GA 주입 후 3분, 10분, 15분의 영상에서 각각 FA $11^{\circ}$$30^{\circ}$ 영상을 획득하였다. 각각의 영상에서 정량적평가와 정성적평가를 한 뒤 독립표본 T검정을 이용하여 통계적 분석을 하였다. 정량적 평가와 정성적 평가 모두 조영제 주입 후 3분과 10분 영상에서 FA $30^{\circ}$ 영상이 FA $11^{\circ}$ 영상보다 약간 우수하였으나 통계적 유의성은 없었다. 그러나 15분 영상에서는 FA $30^{\circ}$ 영상이 FA $11^{\circ}$ 영상보다 통계적으로 유의하게 우수하였다(p<0.05). GA 조영증강 후 15분 MR영상에서 FA $30^{\circ}$ 영상은 기존의 FA $11^{\circ}$ 영상보다 간 병변을 민감하게 검출해낼 수 있다.

A Bacterial Metabolite, Compound K, Induces Programmed Necrosis in MCF-7 Cells via GSK3β

  • Kwak, Chae Won;Son, Young Min;Gu, Min Jeong;Kim, Girak;Lee, In Kyu;Kye, Yoon Chul;Kim, Han Wool;Song, Ki-Duk;Chu, Hyuk;Park, Byung-Chul;Lee, Hak-Kyo;Yang, Deok-Chun;Sprent, Jonathan;Yun, Cheol-Heui
    • Journal of Microbiology and Biotechnology
    • /
    • 제25권7호
    • /
    • pp.1170-1176
    • /
    • 2015
  • Ginsenosides, the major active component of ginseng, are traditionally used to treat various diseases, including cancer, inflammation, and obesity. Among these, compound K (CK), an intestinal bacterial metabolite of the ginsenosides Rb1, Rb2, and Rc from Bacteroides JY-6, is reported to inhibit cancer cell growth by inducing cell-cycle arrest or cell death, including apoptosis and necrosis. However, the precise effect of CK on breast cancer cells remains unclear. MCF-7 cells were treated with CK ($0-70{\mu}M$) for 24 or 48 h. Cell proliferation and death were evaluated by 3-(4,5-dimethylthiazol-2-yl)-2,5-diphenyltetrazolium bromide (MTT) and flow cytometry assays, respectively. Changes in downstream signaling molecules involved in cell death, including glycogen synthase kinase $3\beta$ ($GSK3\beta$), $GSK3\beta$, $\beta$-catenin, and cyclin D1, were analyzed by western blot assay. To block $GSK3\beta$ signaling, MCF-7 cells were pretreated with $GSK3\beta$ inhibitors 1 h prior to CK treatment. Cell death and the expression of $\beta$-catenin and cyclin D1 were then examined. CK dose- and time-dependently inhibited MCF-7 cell proliferation. Interestingly, CK induced programmed necrosis, but not apoptosis, via the $GSK3\beta$ signaling pathway in MCF-7 cells. CK inhibited $GSK3\beta$ phosphorylation, thereby suppressing the expression of $\beta$-catenin and cyclin D1. Our results suggest that CK induces programmed necrosis in MCF-7 breast cancer cells via the $GSK3\beta$ signaling pathway.

PROPERTIES SCUBA-2 850 ㎛ SOURCES AKARI NEP-DEEP FIELD

  • Seo, Hyunjong;Jeong, Woong-Seob;Kim, Minjin;Kim, Seong Jin;Ko, Jongwan;Pyo, Jeonghyun;Kim, Min Gyu;Pearson, Chris;Barrufet, Laia;Varillas, Maria del Carmen Campos;Matsuhara, Hideo;Malkan, Matt;Kim, Helen K.;Takagi, Toshinobu;Miyaji, Takamitsu;Tello, Jorge Diaz;Goto, Tomotsugu;Oi, Nagisa
    • 천문학회지
    • /
    • 제51권3호
    • /
    • pp.49-63
    • /
    • 2018
  • We carry out a study of Sub-Millimeter Galaxies (SMGs) in the AKARI NEP-Deep field using the James Clerk Maxwell Telescope (JCMT) SCUBA-2 $850{\mu}m$ source catalog, released as part of the SCUBA-2 Cosmology Legacy Survey (S2CLS) program. The SCUBA-2 $850{\mu}m$ map has a root mean square (rms) noise of $1.2mJy\;beam^{-1}$ and covers an area of $0.60degree^2$. We find four SMGs which have counterparts to Herschel sources with spectroscopic redshifts in the literature. In addition, three dust obscured galaxies (DOGs) detected in Herschel bands are selected as a comparison sample. We derive IR luminosities of SMGs using the CIGALE code, which are similar to those of high redshift SMGs from previous studies. The contribution of AGN to the total IR luminosity in SMGs (2%-11%) is smaller than the lower limit for the one in DOGs (19%-35%), which is consistent with the expectation from the evolutionary scenario of massive galaxies. We search for SMGs in overdense regions as protocluster candidates and investigate four regions, including candidates around three DOGs. Finally, we argue that follow-up spectroscopic observation for the NEP-Deep field will provide crucial information to understand the role of SMGs in the evolution of massive galaxies.

Development of high yield rice of long grain type adaptable to South-East Asia tropical region

  • Cho, YC;Baek, MK;Park, HS;Nam, JK;Jeong, JM;Kim, WJ;Shin, WC;Song, YC;Cho, JH;Lee, JY;Kim, CS;Park, HG;Kim, BK
    • 한국작물학회:학술대회논문집
    • /
    • 한국작물학회 2017년도 9th Asian Crop Science Association conference
    • /
    • pp.339-339
    • /
    • 2017
  • The long grain rice varieties adaptable to South-east Asia tropical regions were tried to develop in Cambodian Agriculture Research and Development Institute (CARDI), Cambodia. The final goal is to develop rice varieties which can culture in diverse environmental conditions of tropical regions of South-east Asia under climate change. We collected and evaluated for agronomic traits of 131 rice germplasm from Cambodia, China, India, Indonesia, Myanmar, Philippines and Vietnam in CARDI. We selected core germplasm including leading varieties of target countries and made 813 F1 cross combinations between leading varieties of each country and promising germplasm of high yield potential, resistance to biotic/abiotic stresses, aromatic rice, and so on. Out of 607 F1s evaluated to heading date, plant type, agronomic traits, and grain type, 106 F1s selected and advanced to F2 populations. 106 F2 populations were evaluated to major agronomic traits, grain type and yield-component traits, and selected 2,560 plants in 62 F2 populations. During six seasons in 2014~2016, the lines of F3 subsequent-generation were cultured a total of 6,256 lines. In yield trial for promising lines in F5 generation, the growth duration from sowing to harvesting was 97~114 days. These lines were 88~129 in number of grain per panicle, an average of 84.6% in the range of 79.3~91.9% in the percentage of ripened grain and 17.5~22.8g in 1000-brown rice weight. The rough rice yields were in the range of 4.33~6.06 ton/ha with an average of 5.23 ton/ha. The yield was increased to 5~47% than Chulsa and 12~41% than IR66. Five lines, KR54-28-1, KR55-14-2, KR57-5-2, KR67-57-2 and KR128-19-1 were 5.33~6.06 ton/ha in rough rice yield. These high yield potential lines would be evaluated to adaptability in Cambodia, Laos, Myanmar and Vietnam during 2017.

  • PDF

Development of high yield rice of long grain type adaptable to South-East Asia tropical region

  • Cho, YC;Baek, MK;Park, HS;Nam, JK;Jeong, JM;Kim, WJ;Shin, WC;Song, YC;Cho, JH;Lee, JY;Kim, CS;Park, HG;Kim, BK
    • 한국작물학회:학술대회논문집
    • /
    • 한국작물학회 2017년도 9th Asian Crop Science Association conference
    • /
    • pp.155-155
    • /
    • 2017
  • The long grain rice varieties adaptable to South-east Asia tropical regions were tried to develop in Cambodian Agriculture Research and Development Institute (CARDI), Cambodia. The final goal is to develop rice varieties which can culture in diverse environmental conditions of tropical regions of South-east Asia under climate change. We collected and evaluated for agronomic traits of 131 rice germplasm from Cambodia, China, India, Indonesia, Myanmar, Philippines and Vietnam in CARDI. We selected core germplasm including leading varieties of target countries and made 813 F1 cross combinations between leading varieties of each country and promising germplasm of high yield potential, resistance to biotic/abiotic stresses, aromatic rice, and so on. Out of 607 F1s evaluated to heading date, plant type, agronomic traits, and grain type, 106 F1s selected and advanced to F2 populations. 106 F2 populations were evaluated to major agronomic traits, grain type and yield-component traits, and selected 2,560 plants in 62 F2 populations. During six seasons in 2014~2016, the lines of F3 subsequent-generation were cultured a total of 6,256 lines. In yield trial for promising lines in F5 generation, the growth duration from sowing to harvesting was 97~114 days. These lines were 88~129 in number of grain per panicle, an average of 84.6% in the range of 79.3~91.9% in the percentage of ripened grain and 17.5~22.8g in 1000-brown rice weight. The rough rice yields were in the range of 4.33~6.06 ton/ha with an average of 5.23 ton/ha. The yield was increased to 5~47% than Chulsa and 12~41% than IR66. Five lines, KR54-28-1, KR55-14-2, KR57-5-2, KR67-57-2 and KR128-19-1 were 5.33~6.06 ton/ha in rough rice yield. These high yield potential lines would be evaluated to adaptability in Cambodia, Laos, Myanmar and Vietnam during 2017.

  • PDF

폴리피롤 막으로 변성시킨 유리질 탄소 및 백금 전극에서 Cr(Ⅵ) 이온의 정량 (Determination of Cr(Ⅵ) by Glassy Carbon and Platinum Electrodes Modified With Polypyrrole Film)

  • 유광식;우상범;정지영
    • 대한화학회지
    • /
    • 제43권4호
    • /
    • pp.407-411
    • /
    • 1999
  • 본 연구에서는 유리질 탄소전극과 백금 전극의 표면에 폴리피롤 막을 도포 시킨 PPy/GC 및 PPy/Pt 변성전극을 제조하고, 이들 변성 전극들을 작업전극으로 구성한 3-전극 장치를 이용하여 Cr(VI)의 정량분석을 시도하였다. 변성전극들은 +1.0V∼-1.0V를 50 mV/sec로 전위를 걸어주어 순환 전압 전류법으로 쉽게 제조할 수 있었으며, 26회 반복 주사함으로써 연구에 필요한 막의 두께를 조절하였다. PPy/GC 변성전극에서 Cr(VI)의 환원 반응은 +0.6V∼-0.5V(vs. Ag/AgCl)까지 넓은 범위에서 환원되는 경향을 보였으며,-0.25V(vs.Ag/AgCl)의 전위에서 최대 환원 봉우리를 가짐을 알 수 있었다. 이 전위에서 검량곡선을 조사한 결과, 0.1 ppm에서 60.0 ppm의 농도범위에서 기울기가 1.75 mA/ppm이고, 상관계수가 0.998인 좋은 직선관계를 가졌다. PPy/Pt 변성전극에서도 Cr(VI)의 환원 거동은 PPy/GC 변성전극과 유사하였으며, 검량곡선은 1.0 ppm∼60.0ppm의 농도범위에서 직선관계를 가졌다. 이때의 기울기와 상관계수는 각각 0.5 mA/ppm 및 0.923이었다. 그러나 선택성은 PPy/GC 변성전극이 약 3 배정도 우수하였다. PPy/GC 변성전극에서 Cu(II), As(III), pb(II) 및 Cd(II)등은 환원 경향을 보이지 않았으므로, Cr(VI)의 정량분석에는 방해하지 않았다.

  • PDF