Serum levels of FLc were determined in 5 pre-HD CRF patients, 63 CRF patients receiving HD therapy, 15 CAPD and 40 healthy volunteers. The highest serum FLc concentration was observed in patients receiving HD. Concentrations of kappa- and lambda FLc were higher than normal in patients with CRF, and were about 4-fold and 1.8 fold greater than control values in HD patients, with a predominance of lambda chains. This HD-associated elevation of serum FLc strongly suggests a role for FLc in the etiology of light chain deposit disease and AL-amyloidosis. Lambda-FLc and beta 2-m exhibited similar patterns of change in the serum during the course of HD therapy. Further studies may reveal other pathological conditions other than CRF in which these polypeptides may play a role.
We report on time-resolved CCD photometry of four outbursts of a short-period SU UMa-type dwarf nova, V844 Herculis. We successfully determined the mean superhump periods to be 0.05584(64) days, and 0.055883(3) for the 2002 May superoutburst, and the 2006 April-May superoutburst, respectively. During the 2002 October observations, we confirmed that the outburst is a normal outburst, which is the first recorded normal outburst in V844 Her. We also examined superhump period changes during 2002 May and 2006 April-May superoutbursts, both of which showed increasing superhump period over the course of the plateau stage. In order to examine the long-term behavior of V844 Her, we analyzed archival data over the past ten years since the discovery of this binary. Although photometry is not satisfactory in some superoutbursts, we found that V844 Her showed no precursors and rebrightenings. Based on the long-term light curve, we further confirmed V844 Her has shown almost no normal outbursts despite the fact that the supercycle of the system is estimated to be about 300 days. In order to explain the long-term light curves of V844 Her, evaporation in the accretion disk may play a role in the avoidance of several normal outbursts, which does not contradict with the relatively large X-ray luminosity of V844 Her.
The silanols on the surface of silica gel were chlorinated and a phenyl group was introduced onto the silica gel (Remark: Graphics omitted.) by phenylating with phenyllithium. The surface group was derived to a structure similar to Sudan I by nitration, reduction, diazotization, and coupling (with 2-naphthol). The prepared pigment showed approximately the same color as Sudan I, and had very good resistance to water.
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