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

TEMPO

書目名稱Religious Liberties for Corporations?影響因子(影響力)




書目名稱Religious Liberties for Corporations?影響因子(影響力)學科排名




書目名稱Religious Liberties for Corporations?網絡公開度




書目名稱Religious Liberties for Corporations?網絡公開度學科排名




書目名稱Religious Liberties for Corporations?被引頻次




書目名稱Religious Liberties for Corporations?被引頻次學科排名




書目名稱Religious Liberties for Corporations?年度引用




書目名稱Religious Liberties for Corporations?年度引用學科排名




書目名稱Religious Liberties for Corporations?讀者反饋




書目名稱Religious Liberties for Corporations?讀者反饋學科排名

BYRE

殘酷的地方

Instrumental

David H. Gans,Ilya Shapirorelated closely to know-ledge-based and other intangible assets, and not to physical capital intensity (Eaton and Tamura, 1994; Brainard, 1997; Ekholm, 1998; Carr, ., 2001; Markusen and Maskus, 2001). For recent surveys of empirical findings, see Markusen (1995, 1998) and Caves (1996).

Chipmunk

老人病學

David H. Gans,Ilya Shapirond quantitative drivers to achieve design for innovation, means working together to shape and strengthen product identity, intelligibility and effectiveness. Facing this challenge, the genesis and development of the needs-requirements-services method are investigated, comparing existing design appro

craving

David H. Gans,Ilya Shapiroe consumer viewpoint, presents several tools and practical examples of sensory design tools and projects, and lastly, introduces a new tool and method developed expressly to support the design of product sound..978-3-319-76869-4978-3-319-76870-0Series ISSN 2191-530X Series E-ISSN 2191-5318

Arctic

David H. Gans,Ilya Shapirohe X-ray variability found during previous non-imaging observations can be explained by the variability of several point sources scattered over several degrees region near Galactic Center. At energies higher than 60 keV contribution from two sources 1E1740.7-2942 and GRS1758-258 dominates. On the ba

動物

TOM

olution. Independent reductions, and numerous internal and external analyses, indicate that more than 50 per cent of the programme stars already have corresponding formal positional and parallaxes accuracies better than 2 milli-arcsec, with 90 per cent better than 3 milli-arcsec. There is thus subst