2,480 research outputs found

    Incentives to Air Pollution Control

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    Gynäkomastie

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    Magersucht

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    Exophthalmus

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    Kleinwuchs, Großwuchs

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    Fettsucht

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    A Study of Two Early Theologians at Drew Theological Seminary: Randolph S. Foster and John Miley

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    In all branches of learning there is a perennial need to check-up on material to determine if progress is being made and to note where a dead-end has been reached or actual retrogression has taken place. In no field is this check-up more necessary than in the field of theology and philosophy. The problem of this study has been to determine if Arminian theology in America, as represented by two of her most influential theologians, has been true to the philosophy and theology of John Wesley and, also, to determine if they have advanced this thought in any significant manner. More generally the problem of this study has been to delineate the main current of Wesleyan-Arminian theology. Randolph s. Foster and John Miley, consecutively professors of theology at Drew Theological Seminary in the latter half of the nineteenth century, were chosen as representing the most influential school of Arminian theology in America. In this study, comparison has continually been made of the chosen American representatives with the three most influential British theologians, Wesley, Watson, and Pope.

    The Historical and Grammatical Interpretations of John Chrysostom Evaualting on the Basis of his Homilies on Romans

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    In view of the fact that the School of Antioch made no little contribution to the history of interpretation and that its hermeneutical principles are relevant to current problems or the Church, a brief study of the historical and grammatical interpretation of John Chrysostom, the most successful representative of the School of Antioch, may be of some value to pastors who wish to preserve the Church from error and to present the Gospel of Christ in all its truth and power. It is the purpose of this paper, therefore, to outline the hermeneutical principles of John Chrysostom and to show how they came to be what they were. It is to indicate the methods or his historical and grammatical interpretation particularly on the basis of his homilies on the epistle to the Romans. It seeks to evaluate Chrysostom\u27s hermeneutical principles rather than the specific results of his exegesis

    Project Lyman

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    We explore the design of a space mission, Project Lyman, which has the goal of quantifying the ionization history of the universe from the present epoch to a redshift of z ~ 3. Observations from WMAP and SDSS show that before a redshift of z >~ 6 the first collapsed objects, possibly dwarf galaxies, emitted Lyman continuum (LyC) radiation shortward of 912 A, reionizing most of the universe. How LyC escapes from galactic environments, whether it induces positive or negative feedback on the local and global collapse of structures, and the role played by clumping, molecules, metallicity and dust are major unanswered theoretical questions, requiring observational constraint. Numerous intervening Lyman limit systems, which frustrate the detection of LyC from high z objects, thin below z ~ 3 where there are a few objects with apparently very high fesc. At low z there are only controversial detections and a handful of upper limits. A wide-field multi-object spectroscopic survey with moderate spectral and spatial resolution can quantify fesc within diverse spatially resolved galactic environments over redshifts with significant evolution in galaxy assemblage and quasar activity. It can also calibrate LyC escape against Ly-alpha escape, providing an essential tool to JWST for probing the beginnings of reionization. We present calculations showing the evolution of the characteristic apparent magnitude of star-forming galaxy luminosity functions at 900 A, as a function of redshift and assumed escape fraction to determine the required aperture for detecting LyC. We review our efforts to build a pathfinding dual order multi-object spectro/telescope with a (0.5deg)^2 field-of-view, using a GSFC microshutter array, and crossed delay-line micro-channel plate detector.Comment: SPIE oral paper 7011-76 presented at Astronomical Telescopes 2008 - 23 -- 28 June Marseille, France, 12 page, 5 figure
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