An X-Ray Detection Possibility of Star-Formation-Bursting Proto-Elliptical Galaxies

A possibility to detect X-rays from star-formation burst activities in proto-elliptical galaxies is considered. The X-ray flux of an emission due to inverse Compton scattering of the cosmic microwave background (CMB) by high energy electrons accelerated in SNRs is shown to increase as z increases far beyond unity, since the local CMB flux largely increases in association with a z-increase. The flux is estimated for the case of a very high rate of type II supernovae at an initial star formation burst of a proto-elliptical galaxy and is found to be detectable with a future large X-ray telescope such as intended in the XEUS mission.Comment: 4 pages, 1 figure, will appear in PAS

A Variable Partial Covering Model for the Seyfert 1 Galaxy MCG-6-30-15

We propose a simple spectral model for the Seyfert 1 Galaxy MCG-6-30-15 that can explain most of the 1 - 40 keV spectral variation by change of the partial covering fraction, similar to the one proposed by Miller et al. (2008). Our spectral model is composed of three continuum components; (1) a direct power-law component, (2) a heavily absorbed power-law component by mildly ionized intervening matter, and (3) a cold disk reflection component far from the black hole with moderate solid-angle ({\Omega}/2{\pi} \approx 0.3) accompanying a narrow fluorescent iron line. The first two components are affected by the surrounding highly ionized thin absorber with N_H \approx 10^{23.4}cm-2 and log {\xi} \approx 3.4. The heavy absorber in the second component is fragmented into many clouds, each of which is composed of radial zones with different ionization states and column densities, the main body (N_H \approx 10^24.2cm-2, log {\xi} \approx 1.6), the envelope (N_H \approx 10^22.1cm-2, log {\xi} \approx 1.9) and presumably a completely opaque core. These parameters of the ionized absorbers, as well as the intrinsic spectral shape of the X-ray source, are unchanged at all. The central X-ray source is moderately extended, and its luminosity is not significantly variable. The observed flux and spectral variations are mostly explained by variation of the geometrical partial covering fraction of the central source from 0 (uncovered) to \sim0.63 by the intervening ionized clouds in the line of sight. The ionized iron K-edge of the heavily absorbed component explains most of the seemingly broad line-like feature, a well-known spectral characteristic of MCG-6-30-15. The direct component and the absorbed component anti-correlate, cancelling their variations each other, so that the fractional spectral variation becomes the minimum at the iron energy band; another observational characteristic of MCG-6-30-15 is thus explained.Comment: Accepted to Publications of the Astronomical Society of Japa

A light and electron microscopic study of the distribution of gold sodium thiomalate in the rheumatoid synovial membranes

The synovial membranes from 16 rheumatoid patients treated with intramuscular injections of gold sodium thiomalate were observed by light and electron microscopy with special reference to the distribution of gold particles in the tissue. 1) Light microscopic study revealed that the gold demonstrated as cytoplasmic granules by OKAMOTO'S histochemical method were contained in the synovial lining cells and in the macrophages around lymph-follicles and blood vessels in the subsynovial layer. In the well-developed villi on the surface of rheumatoid synovial membrane, large macrophages with gold granules infiltrated into the lymphoid cell accumulation of small lymph-follicles. 2) The deposition of gold in the synovial tissue increased with the increase of the doses of gold administered. 3) Electron microscopic observation indicated that gold particles are contained in the numerous lysosomes in the Type A and intermediate lining cells. The macrophages around lymph-follicles and blood vessels also possessed a large amount of gold particles gathered in the lysosomes of these cells. 4) Macrophages containing gold particles in their long cytoplasmic extensions were found often in a close contact with plasma cells of various differentiation stages. A direct cytoplasmic connection was observed between the two kinds of cells but an artifact could not be excluded. 5) The effect of gold salt in the treatment of RA was discussed from the immunological view point.</p

Transient jet ejections associated with limit-cycle behaviors in the very high state of black hole binaries

Ejection mechanism of transient relativistic jets from black hole binaries is studied. Based on the observations of the limit-cycle behaviors of the superluminal jet source, GRS 1915+105, we infer that the transient jet ejections could happen just after the slim disk emerging from the standard disk at some distance runs over the standard disk and reaches the vicinity of the central black hole. The standard disk releases about a half of the gravitational energy in the course of the accretion, but the released radiative energy could be absorbed by the optically thick slim disk covering the standard disk in this situation. Then, since the inward motion of the slim disk is much faster than that of the standard disk, a quantity of energy released by an amount of gas in the standard disk is received by the much smaller amount of gas in the slim disk. As the result, the energy per mass received by the slim disk is expected to be largely amplified and is estimated to get highly relativistic. Since the energy is much larger than the gravitational energy, the height of the slim disk could significantly increase. Hence, the innermost part of the slim disk from which almost all the angular momentum has been transferred outward could have a much larger height than the black hole size and collide with one another around the central axis of the disk, turning to an outward flow along the axis normal to the disk plane. The flow in this direction can be approximated to be that through the de Laval nozzle and could become supersonic near the distance where the flow has the smallest cross section.Comment: accepted to PAS

Pannus tissue at the cartilage-synovium junction in rheumatoid arthritis.

The cartilage-synovium junction of knees afflicted with rheumatoid arthritis was observed light microscopically using formalin-fixed, decalcified and immunohistochemically stained tissues. Decalcification had little or no influence on immunoreactivity for lysozyme and S-100 protein. All the specimens had pannus formation, which was classified into four types: A) cellular pannus with homogeneous cell pattern, B) cellular pannus of inflammatory cells, C) fibrous pannus with many fibrous bundles, D) fibrous pannus including round cells with scattered fibrous bundles. Type A pannus may be responsible for extensive cartilage degradation, and may occur at the first stage of pannus formation. Type B pannus may occur afterwards, and may be followed by type C pannus at a later stage. Type D pannus was found in two out of 19 specimens. Round cells in type D were positive for S-100 protein and lysozyme, and were probably chondrocytes. The findings indicated that chondrocytes were responsible for cartilage degradation and pannus formation.</p