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Titlebook: Religious Liberties for Corporations?; Hobby Lobby, the Aff David H. Gans,Ilya Shapiro Book 2014 Palgrave Macmillan, a division of Nature A

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tries to most productive use. According to the United Nations’ . (United Nations, 2000), over 63 000 parent companies world-wide have established about 690 000 foreign affiliates in countries other than their own, with the amount of inward FDI stock valued at roughly US$4800 billion in 1999. These f
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David H. Gans,Ilya Shapiroy as part of the macroeconomic theory of capital flows. The foreign investment ‘regime’ (that is, restricted, liberal) could, of course, affect trade in this view, but only through changing the host country’s capital stock. This conceptual approach to direct investment began to break down in the 198
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David H. Gans,Ilya Shapirobustible mixtures. Recently, it has been focused that applications of detonations for aerospace thrusters and industrial machineries, because detonations are able to obtain high enthalpy gases and pressure gains in a simple way. As one of another application, there is the driving source of an experi
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David H. Gans,Ilya Shapiroant, comprehensible, sustainable and shareable solutions. The design research attitude to approach problems in terms of setting and not only solving now suggests that the sounds made by products could be one of the next design challenges in order to try to achieve these results. This chapter investi
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David H. Gans,Ilya Shapiroceptance by consumers. It is of interest to designers, researchers, R&D departments, marketing experts and industries involved in the exploration of the new frontiers now offered by sound. We are all immersed in an intangible world of sounds; however, the fact that only an infinitesimal part of the
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David H. Gans,Ilya Shapiroobtained high angular resolution (~ 5 ÷ 15 arcminutes) images of this region over broad energy band from 3 to 1000 keV. No evidence for presence of supermassive black hole (AGN-like) at the dynamic center of our Galaxy has been found in these observations. The contribution of central few tens of par
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David H. Gans,Ilya Shapiroargets have been observed, with the resulting data filling 500 Gbytes of the HST archives at the ST ScI, ST ECF, and CADC. Even with their much publicized spherical aberration, the HST optics have yielded optical and UV images of unsurpassed resolution. The ring about SN 1987A, the environs of NGC 1
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th consumables for up to a year of further observations. It is yielding high precision astrometric and photometric data for 120 000 pre-selected programme stars, and lower precision astrometric and two-colour photometric data for more than a million stars, typically brighter than 12 mag. The five as
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