In vivo assessment of specific cytotoxic T lymphocyte killing

The direct killing of target cells by cytotoxic T lymphocytes (CTLs) plays a fundamental role in protective immunity to viral, bacterial, protozoan and fungi infections, as well as to tumor cells. In vivo cytotoxic assays take into account the interaction of target and effector cells in the context of the proper microenvironment making the analysis biologically more relevant than in vitro cytotoxic assays. Thus, the development, improvement and validation of in vivo methods are necessary in view of the importance of the results they may provide. We describe and discuss in this manuscript a method to evaluate in vivo specific cytotoxic T lymphocyte killing. We used as model system mice immunized with human recombinant replication-deficient adenovirus 5 (HAd5) containing different transgenes as the trigger of a CTL-mediated immune response. To these mice, we adoptively transferred syngeneic cells labeled with different vital fluorescent dyes. Donor cells were pulsed (target) or not (control non-target) with distinct CD8 T-cell epitopes, mixed in a 1:1 ratio and injected i.v. into immunized or non-immunized recipient mice. After 18-24h, spleen cells are collected and analysed by flow cytometry. A deviation from the 1:1 ratio of control and target cell populations indicates antigen specific lysis of target cells

A cyclic bipolar wind in the interacting binary V 393 Scorpii

V393 Scorpii is a double periodic variable characterized by a relatively stable non-orbital photometric cycle of 253 d. Mennickent et al. argue for the presence of a massive optically thick disc around the more massive B-type component and describe the evolutionary stage of the system. In this paper, we analyse the behaviour of the main spectroscopic optical lines during the long non-orbital photometric cycle. We study the radial velocity of the donor determining its orbital elements and find a small but significant orbital eccentricity (e = 0.04). The donor spectral features are modelled and removed from the spectrum at every observing epoch using the light-curve model given by Mennickent et al. We find that the line emission is larger during eclipses and mostly comes from a bipolar wind. We also find that the long cycle is explained in terms of a modulation of the wind strength; the wind has a larger line and continuum emissivity at the high state. We report the discovery of highly variable chromospheric emission in the donor, as revealed by the Doppler maps of the emission lines Mg II 4481 and C I 6588. We discuss notable and some novel spectroscopic features like discrete absorption components, especially visible at blue depressed O I 7773 absorption wings during the second half-cycle, Balmer double emission with V/R curves showing 'Z-type' and 'S-type' excursions around secondary and main eclipses, respectively, and H beta emission wings extending up to +/- 2000 km s(-1). We also discuss possible causes for these phenomena and for their modulations with the long cycle.

Magnetic non-destructive evaluation of ruptures of tensile armor in oil risers

Risers are flexible multilayered pipes formed by an inner flexible metal structure surrounded by polymer layers and spiral wound steel ligaments, also known as armor wires. Since these risers are used to link subsea pipelines to floating oil and gas production installations, and their failure could produce catastrophic consequences, some methods have been proposed to monitor the armor integrity. However, until now there is no practical method that allows the automatic non-destructive detection of individual armor wire rupture. In this work we show a method using magnetic Barkhausen noise that has shown high efficiency in the detection of armor wire rupture. The results are examined under the cyclic and static load conditions of the riser. This work also analyzes the theory behind the singular dependence of the magnetic Barkhausen noise on the applied tension in riser armor wires.