By James Matthews
This thesis describes the appliance of a Monte Carlo radiative move code to accretion disc winds in kinds of structures spanning nine orders of importance in mass and measurement. In either situations, the consequences supply vital new insights. On small scales, the presence of disc winds in accreting white dwarf binary platforms has lengthy been inferred from the presence of ultraviolet absorption lines. Here, the thesis indicates that a similar winds may also produce optical emission strains and a recombination continuum. On huge scales, the thesis constructs an easy version of disc winds in quasars that's in a position to explaining either the saw absorption and emission signatures – a very important enhance that helps a disc-wind established unification state of affairs for quasars. Lastly, the thesis additionally encompasses a theoretical research into the identical width distribution of the emission strains in quasars, which unearths a huge problem to all unification scenarios.
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Extra info for Disc Winds Matter: Modelling Accretion and Outflows on All Scales (Springer Theses)
Disc Winds Matter: Modelling Accretion and Outflows on All Scales (Springer Theses) by James Matthews