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STUDY OF CLICK CHEMISTRY: WORKING TOWARDS ‘CLICKING’ A NON-STEROIDAL ANTI-INFLAMMATORY TO AN APOPTOSIS INHIBITOR Q-VD-OPHTesak, Jennifer Lynn 17 May 2012 (has links)
No description available.
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STUDY OF CLICK CHEMISTRY: WORKING TOWARDS ‘CLICKING’ A NON-STEROIDAL ANTI-INFLAMMATORY TO AN APOPTOSIS INHIBITOR Q-VD-OPHTesak, Jennifer Lynn January 2012 (has links)
No description available.
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Effect of the Broad-Spectrum Caspase Inhibitor Q-VD-OPh on Neurodegeneration and Neuroinflammation of Sarin exposed miceShah, Ekta J. 27 August 2014 (has links)
No description available.
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X-ray Observations of Bow Shocks around Runaway O Stars. The Case of ζ Oph and BD+43°3654Toala, Jesus, Oskinova, Lidia M., González-Galán, A., Guerrero, M. A., Ignace, Richard, Pohl, M. 20 April 2016 (has links)
Non-thermal radiation has been predicted within bow shocks around runaway stars by recent theoretical works. We present X-ray observations toward the runaway stars ζ Oph by Chandra and Suzaku and of BD+43°3654 by XMM-Newton to search for the presence of non-thermal X-ray emission. We found no evidence of non-thermal emission spatially coincident with the bow shocks; nonetheless, diffuse emission was detected in the vicinity of ζ Oph. After a careful analysis of its spectral characteristics, we conclude that this emission has a thermal nature with a plasma temperature of T ≈ 2 × 106 K. The cometary shape of this emission seems to be in line with recent predictions of radiation-hydrodynamic models of runaway stars. The case of BD+43°3654 is puzzling, as non-thermal emission has been reported in a previous work for this source.
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Evidence for Radio and X-Ray Auroral Emissions From the Magnetic B-Type Star ρ Oph ALeto, P., Trigilio, C., Leone, F., Pillitteri, I., Buemi, C. S., Fossati, L., Cavallaro, F., Oskinova, L. M., Ignace, R., Krtička, J., Umana, G., Catanzaro, G., Ingallinera, A., Bufano, F., Agliozzo, C., Phillips, N. M., Cerrigone, L., Riggi, S., Loru, S., Munari, M., Gangi, M., Giarrusso, M., Robrade, J. 21 April 2020 (has links)
We present new ATCA multiwavelength radio measurements (range 2.1–21.2 GHz) of the early-type magnetic star ρ Oph A, performed in 2019 March during three different observing sessions. These new ATCA observations evidence a clear rotational modulation of the stellar radio emission and the detection of coherent auroral radio emission from ρ Oph A at 2.1 GHz. We collected high-resolution optical spectra of ρ Oph A acquired by several instruments over a time span of about 10 yr. We also report new magnetic field measurements of ρ Oph A that, together with the radio light curves and the temporal variation of the equivalent width of the He I line (λ = 5015 Å), were used to constrain the rotation period and the stellar magnetic field geometry. The above results have been used to model the stellar radio emission, modelling that allowed us to constrain the physical condition of ρ Oph A’s magnetosphere. Past XMM–Newton measurements showed periodic X-ray pulses from ρ Oph A. We correlate the X-ray light curve with the magnetic field geometry of ρ Oph A. The already published XMM–Newton data have been re-analysed showing that the X-ray spectra of ρ Oph A are compatible with the presence of a non-thermal X-ray component. We discuss a scenario where the emission phenomena occurring at the extremes of the electromagnetic spectrum, radio and X-ray, are directly induced by the same plasma process. We interpret the observed X-ray and radio features of ρ Oph A as having an auroral origin.
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Synthesis of Isatin Derivatives Used for the Inhibition of Pro-Apoptotic Jurkat T CellsClay, Charles Michael 16 September 2011 (has links)
No description available.
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