T:raumat ic eosinophili c granuloma(TEG) of the oral mucosa is considered to be a reactive benign lesion. which commonly manifests as an ulcer with elevated and indurated borders Clinically, this lesion simulates a malignant tumor. Histology shows a diffuse. dense, polyrnorphic, and eosinophil - rich cellular infiltra te. which extends deeply into the underlying soft t issues. A major constituent of infil trates is a population of mitotically active‘ la rge‘ atypi cal mononuclear cells. Immunohistologic evaluation of the large atypical cells has suggested a myofibroblastic 01' his tiocytic ol'igin. However, recent reports have shown that these cells are positive 1'01' CD30 antigen and it has been s llggested tha t a subset of TEG cOllld be included within the spectrum of CD30+ lymphoprolifer ative disorders. We have described 2 patients who had oral mllcosal lesions with features of TEG. ln patient 1. the lesiona l cells expressed CD3 .. CD43, LCA. Interestingly, the large cells were strongly CD30 positive. bl1t nega tive for CD68, CD45Ro‘ CD56, CD20. This case was interpreted as a CD30+ Iymphoproliferative disorder. In pa tient 2‘ t he la rge cell s showed strong posit ive for CD68, hut negative for CD30 The small lymphocytic cells ex prerssed CD3 This case was interpreted as an atypical histiocytic granuloma. Therefore, TEGs inclllde atypical histiocytic granllloma a long with the CD30+ lymphoid lesions. These findings suggested that TEG w0111d be a hete rogenous category of oral mucosal di sorders

The conductances of trimethyltetradecylammonium bromide (TTAB) plus triphenyltetradecyl phosphonium bromide (TTPB) and TTAB plus trimethylhexadecylammonium bromide (HTAB) over the entire mole fraction range of TTAB were measured in water and in cyclodextrin plus water mixtures at fixed 4 and 8 mM of cyclodextrin at 30℃. The conductivity plot for both binary mixtures shows a single break from which the mixed critical micelle concentration and degree of micelle ionization were computed. From the slope of the conductivity curve, the equivalent ionic conductivities of the monomeric, associated, and the micelle states were calculated and discussed with respect to the surfactant-cyclodextrin complexation in the whole mole fraction range of both surfactant binary mixtures. The association constant K between the respective monomeric surfactant and cyclodextrin cavity of fixed 4 mM cyclodextrin was computed by considering 1:1 association from the surface tension measurement. A comparison among the K values for HTAB-cyclodetrin, TTAB-cyclodextrin, and TTPB-cyclodextrin shows that the former complexation is significantly stronger in comparison to the other ones due to the longer hydrophobic tail.

Phytoestrogens display estrogen-like activity because of their structural similarity to human estrogens and exhibit high affinity binding for the estrogen receptors (ERs). The prevalence of phytoestrogens in our diets and the biological effects that they

Chop molding composites and 2D carbon/carbon composites were manufactured by hot press molding method. Phenol resin of novolac type was used for matrix precursor and PAN-based carbon, PAN-based graphite and pitch-based carbon fiber were used for reinforcement and boron oxide was used for oxidation retardant. All of the composites were treated by 2000℃ and 2400℃ graphitization process, respectively. After graphitization process, amount of a boron residue in carbon/carbon composites is much according to irregularity of used raw materials. Under the presence of boron in carbon/carbon composites, catalytic effect of boron was a little at 2000℃ graphitization temperature. However, it was quite at 2400℃ graphitization.

P-Cygni type Lyα from starburst galaxies, either nearby galaxies or Lyman Break galaxies, are believed to be formed by galactic outflows such as galactic supershells or galactic superwinds. We develope a Monte Carlo code to calculate the Lyα line transfer in a galactic supershell which is expanding and formed of uniform and dusty neutral hydrogen gas. The escape of Lyα photons from the system is achieved by a number of back-scatterings. A series of emission peaks are formed by back-scatterings. When we observe P-Cygni type Lyα emissions of starforming galaxies, we can usually see merely singly-peaked emission. Hence the secondary and the tertiary emission humps should be destroyed. In order to do this, dust should be spatially more extended into the inner cavity than neutral supershell. We find that the kinematic information of the expanding supershell is conserved even in dusty media. We discuss the astrophysical applications of our results.