• 제목/요약/키워드: lC clusters

검색결과 62건 처리시간 0.025초

The Patterns of Vowel Insertion in Korean Speakers' Production of English C+/l/ and C+/r/ Clusters

  • Kang, Seo-Yoon
    • 말소리와 음성과학
    • /
    • 제4권4호
    • /
    • pp.3-17
    • /
    • 2012
  • This study examines Korean speakers' production of English consonant clusters, focusing on vowel insertion. An acoustic analysis along with a statistical test was carried out to see what factors are involved in this production. The following factors were considered in the present study: phonetic properties, L1 transfer, and cluster types. Specifically, liquid types were considered to see if they cause any difference depending on C+/l/ or C+/r/ clusters in the onset in terms of vowel insertion patterns. That is, it was examined which Korean speakers produce better, C+/l/ or C+/r/ clusters. Interestingly, the result of the present experiment shows that the correct answer percent was higher in the C+/r/ onset clusters than C+/l/ onset clusters unlike Eckman's (1977) Marked Differential Hypothesis. In other words, the occurrence of the vowel insertion in C+/l/ clusters is higher than C+/r/ onset clusters. This may be attributed to L1 transfer. Furthermore, in the present study, three patterns of vowel insertion in the C+/l/ clusters were identified by implementing an acoustic analysis based on vowel duration and formant: a) vowel insertion with gemination, b) phonological epenthesis, and c) phonetic intrusion. However, phonetic intrusion mainly occurred in the C+/r/ clusters. Data were collected from 54 Korean speakers to see what factors are involved in vowel insertion patterns in the production of English consonant clusters. This study provides evidence for L1 transfer, the duration effect of /l/ in a different context, and three kinds of vowel insertion patterns in conjunction with gestural coordination by age groups.

영어 lC 자음군에 관한 역사적 조명과 음운적 고찰 (A phonological study and historical view on IC clusters in English)

  • 오관영
    • 영어어문교육
    • /
    • 제16권4호
    • /
    • pp.201-222
    • /
    • 2010
  • The purpose of this study is to investigate /l/-deletion in lC clusters which are composed of a lateral followed by consonants at syllable-final position in English. For this, I have analyzed /l/-deletion in words depending on conditions and theoretical analyses such as Sonority Sequencing Generalization, Cluster Simplification, Complex sounds and merger, and Feature Geometry, but they didn't offer a very satisfactory explanation to the phenomenon. Therefore, I adopted a historical approach in order to determine the cause and origin of /l/-deletion in lC clusters, and then as a phonological analysis tool, I relied on the constraints and their ranking in Optimal Theory framework for explaining /l/-deletion in the clusters more consistently. As a result, I can explain the phenomenon more explicitly than from the above mentioned analyses.

  • PDF

CORRELATION FUNCTIONS OF THE ABELL, APM, AND X-RAY CLUSTERS OF GALAXIES

  • LEE SUNGHO;PARK CHANGBOM
    • 천문학회지
    • /
    • 제35권3호
    • /
    • pp.111-121
    • /
    • 2002
  • We have measured the correlation functions of the optically selected clusters of galaxies in the Abell and the APM catalogs, and of the X-ray clusters in the X-ray-Brightest Abell-type Clusters of galaxies (XBACs) catalog and the Brightest Clusters Sample (BCS). The same analysis method and the same method of characterizing the resulting correlation functions are applied to all observational samples. We have found that the amplitude of the correlation function of the APM clusters is much higher than what has been previously claimed, in particular for richer subsamples. The correlation length of the APM clusters with the richness R $\ge$ 70 (as defined by the APM team) is found to be $r_0 = 25.4_{-3.0}^{+3.1}\;h^{-1}$ Mpc. The amplitude of correlation function is about 2.4 times higher than that of Croft et al. (1997). The correlation lengths of the Abell clusters with the richness class RC $\ge$ 0 and 1 are measured to be $r_0 = 17.4_{-1.1}^{+1.2}$ and $21.0_{-2.8}^{+2.8}\;h^{-1}$ Mpc, respectively, which is consistent with our results for the APM sample at the similar level of richness. The richness dependence of cluster correlations is found to be $r_0= 0.40d_c + 3.2$ where $d_c$ is the mean intercluster separation. This is identical in slope with the Bahcall & West (1992)'s estimate, but is inconsistent with the weak dependence of Croft et al. (1997). The X-ray bright Abell clusters in the XBACs catalog and the X-ray selected clusters in the BCS catalog show strong clustering. The correlation length of the XBACs clusters with $L_x {\ge}0.65{\times} 10^{44}\;h^{-2}erg\;s^{-1}$ is $30.3_{-6.5}^{+8.2}\;h^{-1}$ Mpc, and that of the BCS clusters with $L_x {\ge}0.70{\times} 10^{44}\;h^{-2}erg\;s^{-1}$ is $30.2_{-8.9}^{+9.8}\;h^{-1}$ Mpc. The clustering strength of the X-ray clusters is much weaker than what is expected from the optical clusters.

Whole genome sequence analysis of Ligilactobacillus agilis C7 isolated from pig feces revealed three bacteriocin gene clusters

  • Jeong Min, Yoo;Remilyn M., Mendoza;In-Chan, Hwang;Dae-Kyung, Kang
    • Journal of Animal Science and Technology
    • /
    • 제64권5호
    • /
    • pp.1008-1011
    • /
    • 2022
  • We here report the whole genome sequence of Ligilactobacillus agilis C7 with anti-listerial activity, which was isolated from pig feces. The genome size of L. agilis C7 (~ 3.0 Mb) is relatively larger compared with other L. agilis strains. L. agilis C7 carries three bacteriocin gene clusters encoding garvicin Q, salivaricin A, and Blp family class II bacteriocin. Garvicin Q and salivaricin A are reported to be active against Listeria monocytogenes and Micrococcus luteus, respectively, as well as against other Gram-positive bacteria. Meanwhile, the bacteriocin encoded in the blp cassette was shown to be active against pneumococci, mediating intraspecies competition. This report highlights the potential of L. agilis C7 for the production of bacteriocins inhibiting pathogenic bacteria.

벼(oryza sativa L.)에서 분리한 Methylotrophic N2-Fixing Bacteria의 형태학적 특성 (Phenotypic Characterization of Methylotrophic N2-Fixing Bacteria Isolated from Rice (Oryza sativa L.))

  • ;박명수;이형석;김충우;이규희;;사동민
    • 한국토양비료학회지
    • /
    • 제37권1호
    • /
    • pp.46-53
    • /
    • 2004
  • 벼(Oryza sativa L.)에 서식하고 있는 메탄올 자화세균(methylotrophic bacteria)의 군집구조를 분석하기 위하여, 국내 3지역(청원, 익산, 밀양)의 경작지 논에서 재배되고 있는 4품종(일미, 동진, 남평, 오대) 벼의 잎, 줄기, 이삭, 뿌리 및 근권토양을 수집하였다. Methanol이 유일한 탄소원으로 첨가된 선택배지를 이용하여, 분홍색 색소체를 갖는 35균주와 무색소체의 5균주를 선별하였으며, 선별균주들의 형태학적, 생리 생화학적 특성을 조사하여 4개의 군집으로 구분하였다. 군집 I 및 IV 는 각각 nitrate와 nitrite reduction 특성에 의해 구별되었으며, pink pigment colony를 형성하는 또 다른 두 개의 군집들은 cellulase 생성유무에 의하여 구분되었다. 표준균주인 Methylobacterium extorquens AM1은 분리균주들과는 다른 군집으로 구분되었으며, M. fujisawaense KACC10744는 III 군집에 속하는 것으로 분석되었다. 분리된 모든 균주들은 urease, oxidase, catalase, pectinase 활성시험에서 양성반응을 나타냈으며, indole, MR-VP, $H_2S$, starch, casein 시험에서는 음성반응을 나타내었다. 또한, 모든 분리 균주들의 열 내성은 없었으며, $45^{\circ}C$ 이상에서는 성장하지 못하였다. 군집 I에서 두개의 분리균주가 각각 gelatin 가수분해와 methane 이용능을 나타내었으며, 대부분의 균주들은 탄소원으로 monosaccharides, disaccharide, polyols를 이용하여 성장하였다. 분리 및 선별되어진 균주들 중 6 균주만이 $86.2-809.9nmol\;C_2H_4\;h^{-1}\;mg^{-1}$ protein 범위의 질소고정능을 나타내었다.

THE EVOLUTION OF THE GALACTIC GLOBULAR CLUSTERS.: I. METAL ABUNDANCE CALIBRATIONS

  • Lee, See-Woo;Park, Nam-Kyu
    • 천문학회지
    • /
    • 제17권2호
    • /
    • pp.69-103
    • /
    • 1984
  • Five different calibrations of metal abundances of globular clusters are examined and these are compared with metallicity ranking parameters such as $(Sp)_c$, . Q39 and IR-indices. Except for the calibration $[Fe/H]_H$ by the high dispersion echelle analysis. the other calibration scales are correlated with the morphological parameters of red giant branch. In the $[Fe/H]_H$-scale. the clusters later than ${\sim}F8$ have nearly a constant metal abundance. $[Fe/H]_H{\simeq}-1.05$, regradless of morphological characteristics of horizontal branch and red giant branch. By the two fundamental calibration scales of $[Fe/H]_L$ (derived by the low dispersion analysis) and $[Fe/H]_{{\Delta}s}$ (derived by the spectral analysis of RR Lyrae stars). the globular clusters are divided into the halo clusters with [Fe/H]<-1.0 and the disk clusters confined within the galactocentric distance ${\tau}_G=10\;kpc$ and galactic plane distance |z|=3 kpc. In this case the abundance gradient is given by d[Fe/H]/$dr_G{\approx}-0.05\;kpc^{-1}$ and d[Fe/H]/$d|z|{\simeq}-0.08\;kpc^{-1}$ within ${\tau}_G=20\;kpc$ and |z|=10 kpc, respectively. According to these characteristics of the spatial distribution of globular clusters. the chemical evolution of the galactic globular clusters can be accounted for by the two-zone (disk-halo) slow collapse model when the $[Fe/H]_L$-or $[Fe/H]_{{\Delta}s}$-scale is applied. In the case of $[Fe/H]_H$-scale, the one-zone fast collapse model is preferred for the evolution of globular clusters.

  • PDF

애기장대(Arabidopsis thaliana) 현탁배양세포의 원형질체로부터 식물체 재분화 (Plant Regeneration from Protoplasts of Suspension Cultured Cells in Arabidopsis thaliana)

  • 김명덕;김준철;진창덕;임창진;한태진
    • 식물조직배양학회지
    • /
    • 제27권2호
    • /
    • pp.125-131
    • /
    • 2000
  • 원형질체는 현탁배양된 세포괴로부터 1% cellulase R-10, 0.25% pectolyase Y-23, 그리고 0.5% driselase가 포함된 CPD 효소용액에서 4시간의 진탕 (40 rpm)조건에서 쉽게 분리되었다. 분리된 원형질체는 1 mg/L 2,4-D, 0.5 mg/L kinetin , 200 rng/L spermidine 그리고 68 g/L glucose가 포함된 KM 액체배지에서 배양되었으며, 또한 현탁배양중인 동종의 feeder cell이 있는 CP배지 위에 액체배양배지를 1 mL균일하게 퍼트린 후,$25^{\circ}C$, 암조건으로 4주간 양육배양하였다. 원형질체 유래 SF 캘러스는 0.05 mg/L IAA, 7 mg/L 2lip와 30mg/L sucrose가 첨가된 MS 재분화 배지에서 광조건으로 4주동안 배양되었을 때, 60% 이상의 shoot를 형성하였다. 이후, 식물의생장조절물질이 첨가되지 않은 MS 배지로 옮겨 뿌리를 유도하였으며, 재분화된 식물체는 토양으로 옮겨 배양 8주후에 종자를 형성하였다.

  • PDF

김치에서 분리한 Leuconostoc속의 RAPD 법을 이용한 유전적 변이도 추론 (Studies on the Genetic Diversity using RAPD in Leuconostoc sp. Isolated from Kimchi)

  • 김은경;류춘선;소명환;김영배
    • 한국식품과학회지
    • /
    • 제29권5호
    • /
    • pp.1063-1066
    • /
    • 1997
  • 김치에서 분리한 Leuconostoc속 4종 34주를 RAPD-PCR방법으로 분석하여 기존의 동정 결과를 비교 검토하였다. 상사도 0.5이상의 수준에서 L. mesenteroides subsp. mesenteroides 및 L. mesenteroides subsp. dextranicum균주들은 각 각 3 및 2의 cluster를 형성하였고 L. paramesenteroides 및 L. lactis는 각 각 하나의 cluster를 형성하였다. 각 각의 표준 균주들도 같은 종 혹은 아종의 cluster에 속하는 것으로 나타났다. 그러나 a 및 b cluster의 상사도는 0.2 이하의 수준이며 c cluster는 이들과 상사도가 더욱 낮아 L. mesenteroides subsp. mesenteroides 균주들은 유전적 상사도가 낮은 다양한 종류의 집단임을 추정 할 수 있었다.

  • PDF

생약복합물의 지방세포형성억제 기전규명을 위한 전사체 분석 (Transcriptome Analyses for the Anti-Adipogenic Mechanism of an Herbal Composition)

  • 이해용;강련화;배성민;채수안;이정주;오동진;박석원;조수현;심예지;윤유식
    • 생명과학회지
    • /
    • 제20권7호
    • /
    • pp.1054-1065
    • /
    • 2010
  • 생약복합물인 SH21B는 황금(Scutellaria baicalensis Georgi), 행인(Prunus armeniaca Maxim), 마황(Ephedra sinica Stapf), 석창포(Acorus gramineus Soland), 포황(Typha orientalis Presl), 원지(Polygala tenuifolia Willd), 하엽(Nelumbo nucifera Gaertner)의 혼합(비율 3:3:3:3:3:2:2)으로 이루어졌다. SH21B는 예로부터 한의학에서 비만의 치료에 사용되어 왔으나 자세한 분자적 메커니즘과 효능에 대한 연구는 이루어지지 않았다. 본 연구진은 선행연구를 통해 SH21B가 지방세포의 분화에서 adipogenesis (지방세포형성)와 관련된 유전자를 조절하여 중성지방의 축적을 억제함을 밝혔다. 본 연구에서는, microarray 기술을 이용하여 adipogenesis의 in vitro 모델인, 3T3-L1 세포에서 SH21B에 의한 지방세포형성 억제의 분자적 기작을 보다 상세하게 연구하고자 하였다. 전지방세포, 분화된 세포 그리고 SH21B에 의해 분화가 억제된 세포의 각각의 유전자 발현을 분석하기 위해 각 시료들에서 total RNA를 분리하여 cDNA를 합성한 후 microarray에 적용시켰다. 그 결과, 각각의 시료들의 비교에서 2배 이상의 유의한 발현 변화를 가지는 2,568개의 유전자를 확보하였다. 이 유전자들에 대해 Hierarchical clustering과 K-means clustering 분석을 진행하였고 서로 다른 양상을 가지는 9개의 군집(cluster)들을 분류하였다. 그 중, SH21B의 첨가에 의해 뚜렷하게 감소(cluster 4, cluster 6 및 cluster 9)하거나 반대로 뚜렷하게 증가(cluster 7와 cluster 8)하는 양상을 보이는 군집들을 따로 선별하여 그 군집들에 포함되어 있는 유전자들을 분석하였다. 선택 된 5개의 군집에는 지방세포형성과 세포증식에 관련된 유전자가 다수 포함되어 있었다. Cluster 4, cluster 6 그리고 cluster 9에는 peroxisome proliferator activated receptor gamma $\gamma$ ($PPAR{\gamma}$), CCAAT/enhancer binding protein $\alpha$ (C/$EBP{\alpha}$), sterol regulatory element binding transcription factor 1 (SREBF1), adiponectin (ADIPOQ), fatty acid synthase (FASN), lipoprotein lipase (LPL) 등의 지방세포형성 유도 및 관련 인자와 B-cell leukemia/lymphoma6 (BCL6), retinoblastoma 1 (RB1), cyclin-dependent kinase inhibitor 2C (CDKN2c), ras homolog gene family, member B (RHOB) 등의 많은 세포증식 억제 유전자가 포함되었다. 이와는 반대로, cluster 7과 cluster 8에는 $\beta$-catenin, cyclin D1 (CCND1), WNT1 inducible signaling pathway protein 2 (WISP2) 등과 같은 지방 세포형성 억제 조절자와 MARCKS-like1 (MARCKSL1), colony stimulating factor 1 (CSF1), discoidin domain receptor family, member 2 (DDR2), leukemia inhibitory factor receptor (LIFR) 등의 세포증식을 유도하는 조절자가 다수 포함되었다. 결론적으로, 이러한 결과들은 SH21B가 지방세포형성과 관련된 조절자 및 세포증식과 관련 된 조절자들의 유전자 발현을 조절하여 지방세포형성을 억제함을 제시한다.

THE EVOLUTION OF THE GALACTIC GLOBULAR CLUSTERS.: II. HELIUM ABUNDANCES AND AGES

  • Lee, See-Woo
    • 천문학회지
    • /
    • 제18권2호
    • /
    • pp.41-69
    • /
    • 1985
  • For the well observed 16 globular clusters with known metal abundance (Z), the helium abundances (Y) and ages are determined by various methods, and the relations between Y, Z and age are examined. The luminosity $L_{RR}$ of RR Lyrae stars is known to be dependent of evolutionary models and pulsation theory in the sense that the pulsation theory and horizontal branch (HB) models yield the anticorrelation between $L_{RR}$ and Z whereas main sequence (MS) and red giant branch (RGB) models yield the direct correlation between them. Similarly the anticorrelation between Y and Z is obtained from the HB models and pulsation theory whereas the direct correlation between them is obtained when the RGB model is applied. The current evolutionary models yield the anticorrelation between Z and age of clusters whenever the direct correlation between Y and Z holds. However when the anticorrelation between Y and Z is applied for age determination, the similar age of clusters is obtained as shown by Sandage (1982b). The ages, which are determined by the fitting of C-M diagrams to isochrones in the ($M_v$, B-V)-plane, suggest the two different chemical enrichment processes, which could be accounted for by the disk-halo model for the chemical evolution of the Galaxy (Lee and Ann 1981). Also it is known that the R-method is very useful for Y-determination and the derived Y's show the increasing rate of $\frac{{\Delta}Y}{{\Delta}Z}{\simeq}0.5$ which is comparable to the observed value of $\frac{{\Delta}Y}{{\Delta}Z}{\simeq}0.3$ from HII regions and planetary nebulae by Peimbert and Torres-Peimbert (1976). In this case, the age-metallicity relation of globular clusters could be explained by the disk-halo model.

  • PDF