[Preparation and characterization of a monoclonal antibody directed against bovine leukocytes]. / Préparation et caractérisation d'un anticorps monoclonal dirigé contre des leucocytes bovins.

A monoclonal antibody (MAb-M25) was obtained by immunizing BALB/C mice with tumour cells isoled from a familial thymic lymphosarcoma observed in Friesian cattle. The specificity of this MAb was assessed using PBL, lymphoids organs (lymph node, spleen, tonsil, Pleyer's patch) and non lymphoid tissues (liver, skin) from clinical normal cattle. Immunofluorescence and immunohistochemistry methods were used to characterise this monoclonal antibody. It reacted with 27% of peripheral blood lymphocytes and a large proportion of mononuclear cell in the lymphoid organ, in the thymic cortical, in the dermis and in the liver. It also stained lymphocytes of the mantle of follicules and thymocytes of the thymus cortex. The tissue distribution of M25 have a similarity with the human CD1c Mab and the bovine 20-27 MAb.

Preparation and characterization of a monoclonal antibody against bovine CD5 lymphocyte surface antigen.

The M1 monoclonal antibody (mAb) was proved to recognize 51-70% of Bovine peripheral blood lymphocytes (PBL). The M1+ cells were SIg-. In spleen and lymph nodes, the M1 positive lymphocytes were located within the T cell areas. All the lymphoid follicles remained negative. In the thymus, 10% of thymocytes were M1+, most of them were located in the medulla. The M1 mAb did not inhibit spontaneous rosette formation by sheep erythrocytes and bovine lymphocytes. On the other hand, biochemical analysis of membrane antigen with bovine thymic tumor cell line LB203 gave a molecular weight of 75 kDa. Despite a slight difference in biochemical results (75 vs 67-69 kDa). Our data permit us to consider M1 mAb as a possible homologous of human anti-CD5 mAb. Finally, M1 cross-reacted with sheep peripheral blood T lymphocytes.

Immunolabelling of Shiga toxin in macrophages infected with Shigella dysenteriae 1.

Immunolabelling of Shiga toxin in macrophages infected with a non-invasive Shigella dysenteriae 1 isolate showed that bacteria remained alive for 3 h after ingestion within the phagocytic vacuole and synthesized Shiga toxin. The normal process of toxin secretion was, however, impaired by the phagosomal environment and toxin molecules accumulated within the bacterial cytoplasm.

Immunodetection of lipopolysaccharide in macrophages during the processing of non invasive Shigella dysenteriae.

The location of lipopolysaccharide (LPS) was studied by immunofluorescence and immunoelectron microscopy in macrophages infected with a non-invasive Shigella dysenteriae 1 strain. Bacterial degradation began only 3 h after the end of infection. The first visible sign of degradation was detected by immunogold labelling at the level of LPS which detached from the bacterial surface and was transferred to the perinuclear lysosomes. After a few hours, it was found in small vesicles spread over the whole macrophage cytoplasm in which it remained visible for 72 h. These vesicles seemed to belong to a compartment in which slowly or non-degradable compounds are stored. LPS separation from the bacterial surface was immediately followed by the degradation of the intrabacterial constituents. The long lag period observed before initiation of bacterial degradation was not due to a lack of phagosome acidification, since DAMP, a lysosomotropic drug was found in all phagosomes at the end of the ingestion period. The frequency of phagosome-lysosome fusion was 30% for S dysenteriae and 72% for B subtilis used as a reference of high fusion frequency. The low frequency of fusion of S dysenteriae may play an important role in the survival of the virulent strains in macrophage by providing bacteria enough time to lyse the phagosome membrane before lysosome fusion occurs.

Preliminary report of familial thymic lymphosarcoma in Holstein calves.

Seventy-three cases of the thymic form of leukosis were found in Holstein calves in five departments of France over a period of five months. Most of the calves had been sired by the same bull. The calves were negative for specific antibodies to bovine leukaemia virus. Morphological studies including light and electron-microscopic cytology, and serological and virological studies of 14 of the cases suggest that the disease was transmitted genetically.

Imaging photopolarimeter on pioneer saturn.

An imaging photopolarimeter aboard Pioneer 11, including a 2.5-centimeter telescope, was used for 2 weeks continuously in August and September 1979 for imaging, photometry, and polarimetry observations of Saturn, its rings, and Titan. A new ring of optical depth < 2 x 10(-3) was discovered at 2.33 Saturn radii and is provisionally named the F ring; it is separated from the A ring by the provisionally named Pioneer division. A division between the B and C rings, a gap near the center of the Cassini division, and detail in the A, B, and C rings have been seen; the nomenclature of divisions and gaps is redefined. The width of the Encke gap is 876 +/- 35 kilometers. The intensity profile and colors are given for the light transmitted by the rings. A mean particle size less, similar 15 meters is indicated; this estimate is model-dependent. The D ring was not seen in any viewing geometry and its existence is doubtful. A satellite, 1979 S 1, was found at 2.53 +/- 0.01 Saturn radii; the same object was observed approximately 16 hours later by other experiments on Pioneer 11. The equatorial radius of Saturn is 60,000 +/- 500 kilometers, and the ratio of the polar to the equatorial radius is 0.912 +/- 0.006. A sample of polarimetric data is compared with models of the vertical structure of Saturn's atmosphere. The variation of the polarization from the center of the disk to the limb in blue light at 88 degrees phase indicates that the density of cloud particles decreases as a function of altitude with a scale height about one-fourth that of the gas. The pressure level at which an optical depth of 1 is reached in the clouds depends on the single-scattering polarizing properties of the clouds; a value similar to that found for the Jovian clouds yields an optical depth of 1 at about 750 millibars.