Search

Recent unconfirmed literature data suggest that elevated concentrations of the multifunctional cytokine hepatocyte growth factor (HGF) might be a marker of increased incidence of acute rejection after organ transplantation. The aim of this study was to test the hypothesis that HGF levels may correlate with the rejection and/or with the production of HLA and MHC Class I chain-related antigens A (MICA) specific antibodies. Sixty-three heart transplant recipients were included into the study. Hundred and eighty-five endomyocardial biopsies (EMB) obtained up to 6 months after transplantation were retrospectively analyzed for signs of cellular (CR) and antibody-mediated rejection (AMR). Pre- and post-transplant sera were tested for HGF concentrations and antibodies to HLA class I, class II and MICA antigens by xMap technology (Luminex). Pre-transplant HGF did not correlate with the incidence of CR or AMR. However, higher HGF concentrations correlated significantly with HLA antibody production before and after transplantation ( P = 0.006 and P < 0.0001 respectively). Patients with both HLA class I and class II antibodies before transplantation had significantly lower AMR-free survival. Furthermore, recipients with pre-transplant donor-specific antibodies (DSA) had significantly lower AMR-free survival (50%) than recipients without pre-transplant HLA antibodies (90%) and patients with antibodies not specific to donor antigens (92%) ( P = 0.005). Post-transplant MICA antibodies tended to be more frequent in patients with AMR ( P = 0.063). In conclusion, elevated HGF concentrations in our study were not associated with the incidence of CR and/or AMR but with the presence of HLA-specific antibodies. Testing for DSA before heart transplantation by Luminex may be helpful for the identification of patients with increased risk of AMR. [ABSTRACT FROM AUTHOR]

Killer cells immunoglobulin-like receptors (KIRs) are a family of inhibitory and activating receptors expressed mainly by natural killer (NK) cells and few subsets of T lymphocytes. KIRs regulate NK cells’ activity through interactions with specific HLA class I molecules and other yet unknown ligands presented on target cells. At present, 17 KIR genes and pseudogenes have been identified. As the number of KIR genes in different haplotypes varies, a wide range of genotypes in different ethnic populations may be observed. In our study, 125 healthy non-related Czech individuals were KIR typed both by sequence-specific primers and by sequence-specific oligonucleotide KIR genotyping methods. Thirty-eight different genotypes were observed in the Czech population and all 16 KIR genes known to date were found. Framework genes KIR 3DL3, KIR 2DL4, KIR 3DL2 and the pseudogene KIR 3DP1 were present in all individuals. The most frequent non-framework KIR genes detected in the Czech population were: KIR 2DL1 (95%), KIR 3DL1 (94%), KIR 2DS4 (92%) and the pseudogene 2DP1 (94%). Human leucocyte antigen (HLA)-C typing demonstrated prevalence of the C1/C2 heterozygosity (43%) and C1 homozygosity (41%) over the C2 heterozygosity. One hundred and twenty individuals from our panel carried at least one inhibitory KIR for the corresponding HLA-C group found in the genotype. Gene frequencies and found genotypes demonstrated similarity of the Czech population's KIR repertoire with the KIR repertoires of other Caucasian populations studied before. [ABSTRACT FROM AUTHOR]

The formation of Saturn and its disk is simulated using a new N-body self-gravitational model. It is demonstrated that the formation of the disk and the planet is the result of gravitational contraction of a slowly rotated particle cloud that have a shape of slightly deformed sphere. The sphere was flattened by a coefficient of 0.8 along the axis of rotation. During the gravitational contraction, the major part of the cloud transformed into a planet and a minor part transformed into a disk. The thin structured disk is a result of the electromagnetic interaction in which the magnetic forces acting on charged particles of the cloud originate in the core of the planet. The simulation program gives such parameters of Saturn as the escape velocity of about 35 km/s at the surface, density, rotational velocities of the rings and temperature distribution. [ABSTRACT FROM AUTHOR]

A mechanism of formation of a spiral galaxy is proposed. The galaxy is considered to be a cluster consisting of stars and gaseous clouds. Initially, the galaxy has elliptical geometry and slow rotational motion around one axis. The gravitational interaction between the stars has been modelled. The cluster contracted and transformed its geometry. The geometry of the initial cluster changes due to the change of the rotational velocities of the stars in accordance with the Kepler's second law and change of the relative positions of the stars. The computer simulation reveals that a spiral shaped galaxy is a result of the transformation of a cluster of non-spherical symmetry. An example of the gravitational contraction of an elliptically-shaped galaxy is presented in this paper. [ABSTRACT FROM AUTHOR]