Investigation of mechanisms involved in ultraviolet B radiation-induced, T cell -mediated immune suppression

Cutaneous exposure to ultraviolet-B radiation (UVR) results in the suppression of cell-mediated immune responses such as contact hypersensitivity (CHS) and delayed-type hypersensitivity (DTH). This modulation of immune responses is mediated by local or systemic mechanisms, both of which are associated with the generation of antigen-specific suppressor T lymphocytes (Ts). UV-induced Ts have been shown to be CD3+CD4+CD8 − T cells that control multiple immunological pathways. However, the precise mechanisms involved in the generation and function of these immunoregulatory cells remain unclear. We investigated the cellular basis for the generation of UV-induced Ts lymphocytes in both local and systemic models of immune suppression, and further examined the pleiotrophic function of these immunoregulatory cells. ^ We used Thy1.1 and Thy1.2 congenic mice in a draining lymph node (DLN) cell transfer model to analyze the role played by epidermal Langerhans cells in the generation of Ts cells. We demonstrate that T cells tightly adhered to antigen-presenting cells (APC) from UV-irradiated skin are the direct progenitors of UV-induced Ts lymphocytes. Our studies also reveal that UV-induced DNA-damage in the form of cyclobutyl pyrimidine dimers (CPD) in the epidermal APC is crucial for the altered maturation of these adherent T cells into Ts. ^ We used TCR transgenic mice in an adoptive transfer model and physically tracked the antigen-specific clones during immune responses in unirradiated versus UV-irradiated mice. We demonstrate that UV-induced Ts and effector TDTH cells share the same epitope specificity, indicating that both cell populations arise from the same clonal progenitors. UVR also causes profound changes in the localization and proliferation of antigen-specific T cells during an immune response. Antigen-specific T cells are not detectable in the DLNs of UV-irradiated mice after 3 days post-immunization, but are found in abundance in the spleen. In contrast, these clones continue to be found in the DLNs and spleens of normal animals several days post-immunization. Our studies also reveal that a Th2 cytokine environment is essential for the generation of Ts in UV-irradiated mice. ^ The third part of our study examined the pleiotrophic nature of UV-induced Ts. We used a model for the induction of both cellular and humoral responses to human gamma-globulin (HGG) to demonstrate that UV-induced Ts lymphocytes can suppress DTH as well as antibody responses. (Abstract shortened by UMI.) ^

Ionizing radiation and short wavelength UV activate NF-κB through two distinct mechanisms

We examined the mechanisms by which two different types of photonic radiation, short wavelength UV (UV-C) and γ radiation, activate transcription factor NF-κB. Exposure of mammalian cells to either form of radiation resulted in induction with similar kinetics of NF-κB DNA binding activity, nuclear translocation of its p65(RelA) subunit, and degradation of the major NF-κB inhibitor IκBα. In both cases, induction of NF-κB activity was attenuated by proteasome inhibitors and a mutation in ubiquitin-activating enzyme, suggesting that both UV-C and γ radiation induce degradation of IκBs by means of the ubiquitin/proteasome pathway. However, although the induction of IκBα degradation by γ rays was dependent on its phosphorylation at Ser-32 and Ser-36, UV-C-induced IκBα degradation was not dependent on phosphorylation of these residues. Even the “super repressor” IκBα mutant, which contains alanines at positions 32 and 36, was still susceptible to UV-C-induced degradation. Correspondingly, we found that γ radiation led to activation of IKK, the protein kinase that phosphorylates IκBα at Ser-32 and Ser-36, whereas UV-C radiation did not. Furthermore, expression of a catalytically inactive IKKβ mutant prevented NF-κB activation by γ radiation, but not by UV-C. These results indicate that γ radiation and UV-C activate NF-κB through two distinct mechanisms.

The steam fitters' computation and price book; consisting of tables giving the cubical contents of rooms of various sizes, tables giving the number of square feet of wall surface, tables giving the number of square feet of window surface. Tables giving radiation required for rooms of any size at various proportions. Also tables showing the cost of radiation ... Tables giving size, price, weight etc., of pipe, fittings, valves, etc. In addition ... some general information on points of interest to steam and hot water fitters.

At foot of t.-p.: Copyrighted 1893 by Mark Dean; on verso of t.-p. copyright date given 1895.

General discussion session of the 2004 Hume-Rothery Symposium on "The structure and diffusional growth mechanisms of irrational interphase boundaries"

Details on the general discussion session of the 2004 Hume-Rothery Symposium on "The Structure and Diffusional Growth Mechanisms of Irrational Interphase Boundaries" is presented. The symposium was held on Mar 17, 2004 at the Charlotte Convention Center in Charlotte NC.

Pulsar binary systems in a nonsymmetric theory of gravitation II. Dipole radiation

This paper deals with the emission of gravitational radiation in the context of a previously studied metric nonsymmetric theory of gravitation. The part coming from the symmetric part of the metric coincides with the mass quadrupole moment result of general relativity. The one associated to the antisymmetric part of the metric involves the dipole moment of the fermionic charge of the system. The results are applied to binary star systems and the decrease of the period of the elliptical motion is calculated.

H(2) infrared line emission from the ionized region of planetary nebulae

Context. The analysis and interpretation of the H(2) line emission from planetary nebulae have been done in the literature by assuming that the molecule survives only in regions where the hydrogen is neutral, as in photodissociation, neutral clumps, or shocked regions. However, there is strong observational and theoretical evidence that at least part of the H(2) emission is produced inside the ionized region of these objects. Aims. The aim of the present work is to calculate and analyze the infrared line emission of H(2) produced inside the ionized region of planetary nebulae using a one-dimensional photoionization code. Methods. The photoionization code Aangaba was improved in order to calculate the statistical population of the H(2) energy levels, as well as the intensity of the H(2) infrared emission lines in the physical conditions typical of planetary nebulae. A grid of models was obtained and the results then analyzed and compared with the observational data. Results. We show that the contribution of the ionized region to the H(2) line emission can be important, particularly in the case of nebulae with high-temperature central stars. This result explains why H(2) emission is more frequently observed in bipolar planetary nebulae (Gatley's rule), since this kind of object typically has hotter stars. Collisional excitation plays an important role in populating the rovibrational levels of the electronic ground state of H(2) molecules. Radiative mechanisms are also important, particularly for the upper vibrational levels. Formation pumping can have minor effects on the line intensities produced by de-excitation from very high rotational levels, especially in dense and dusty environments. We included the effect of the H(2) molecule on the thermal equilibrium of the gas, concluding that, in the ionized region, H(2) only contributes to the thermal equilibrium in the case of a very high temperature of the central star or a high dust-to-gas ratio, mainly through collisional de-excitation.

Passage of radiation through wormholes of arbitrary shape

We study quasinormal modes and scattering properties via calculation of the S matrix for scalar and electromagnetic fields propagating in the background of spherically symmetric and axially symmetric traversable Lorentzian wormholes of a generic shape. Such wormholes are described by the general Morris-Thorne ansatz. The properties of quasinormal ringing and scattering are shown to be determined by the behavior of the wormhole's shape function b(r) and shift factor Phi(r) near the throat. In particular, wormholes with the shape function b(r), such that b(dr) approximate to 1, have very long-lived quasinormal modes in the spectrum. We have proved that the axially symmetric traversable Lorentzian wormholes, unlike black holes and other compact rotating objects, do not allow for superradiance. As a by-product we have shown that the 6th order WKB formula used for scattering problems of black or wormholes gives quite high accuracy and thus can be used for quite accurate calculations of the Hawking radiation processes around various black holes.