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Reluctant Warriors

Reluctant Warriors

James Matthews

Oxford University Press
2012
sidottu
Reluctant Warriors challenges traditional political interpretations of the Spanish Civil War, and sets it in a new and immediately human light. It is a comparative study of Nationalist Army and Republican Popular Army conscripts, and analyses the conflict from the perspective of those who were involved against their will. While militants on both sides joined the conflict voluntarily, millions of Spanish men coped with the military uprising as an unwanted intrusion into their lives. James Matthews firstly examines the climate in which both sides implemented mass conscription within their zones. He analyses the process of conscription from call-up to placement in a unit, and looks at the methods employed to motivate and maintain the morale of drafted men, as well as the approaches to discipline in the two armies. Finally, he examines situations in which men avoided front line service. These accounted for constant manpower losses on both sides, and were particularly marked for the Republic. Reluctant Warriors reveals that the Nationalist Army managed its conscripted men better than the Republican Popular Army; a vital factor in determining the ultimate outcome of the war.
Back Pain: Natural Solutions To Live Pain-Free - Pain Relief, Home Treatment, Chronic Pain & Sciatica
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Disc Winds Matter

Disc Winds Matter

James Matthews

Springer International Publishing AG
2017
sidottu
This thesis describes the application of a Monte Carlo radiative transfer code to accretion disc winds in two types of systems spanning 9 orders of magnitude in mass and size. In both cases, the results provide important new insights. On small scales, the presence of disc winds in accreting white dwarf binary systems has long been inferred from the presence of ultraviolet absorption lines. Here, the thesis shows that the same winds can also produce optical emission lines and a recombination continuum. On large scales, the thesis constructs a simple model of disc winds in quasars that is capable of explaining both the observed absorption and emission signatures – a crucial advance that supports a disc-wind based unification scenario for quasars. Lastly, the thesis also includes a theoretical investigation into the equivalent width distribution of the emission lines in quasars, which reveals a major challenge to all unification scenarios.
Disc Winds Matter

Disc Winds Matter

James Matthews

Springer International Publishing AG
2018
nidottu
This thesis describes the application of a Monte Carlo radiative transfer code to accretion disc winds in two types of systems spanning 9 orders of magnitude in mass and size. In both cases, the results provide important new insights. On small scales, the presence of disc winds in accreting white dwarf binary systems has long been inferred from the presence of ultraviolet absorption lines. Here, the thesis shows that the same winds can also produce optical emission lines and a recombination continuum. On large scales, the thesis constructs a simple model of disc winds in quasars that is capable of explaining both the observed absorption and emission signatures – a crucial advance that supports a disc-wind based unification scenario for quasars. Lastly, the thesis also includes a theoretical investigation into the equivalent width distribution of the emission lines in quasars, which reveals a major challenge to all unification scenarios.