Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/9626
Title: Investigating the Soft X-ray Background of the Milky Way
Authors: Supper, Michelle Abbie
Supervisors: Raine, Derek
Award date: 1-Jul-2011
Presented at: University of Leicester
Abstract: This thesis uses the data from twenty ROSAT and XMM observations to investigate the structures that generate the soft X-ray background of the Milky Way. Ten of these observations lie in the direction of the Loop 1 Superbubble, specifically, within the North Polar Spur, the Northern Bulge, and immediately south of the Galactic Plane. The others are located in the Anti-centre direction, where the X-ray background is less complex. Using a novel processing technique, point sources and enhancements were successively removed from the observations until only the Diffuse X-ray Background (DXRB) re¬mained. By modelling the spectra of this clean data, and separately analysing the 0 and 0 viii emission lines, the various structures in the DXRB were identified, and their properties determined. The resulting models strongly indicate the existence of three previously unidentified components: a 14 pc thick, 0.1 keV shell surrounding Loop I, an inhomogeneous 0.25 keV Galactic Halo, and a non-thermal component present in the Galactic Centre direction. In contrast with previous work, no evidence was found for a cool Galactic Halo. The centre of Loop I was placed 290 pc away, 80 pc farther than previously believed. Additionally, an ongoing interaction was discovered between the Local Hot Bubble and Loop I.
Links: http://hdl.handle.net/2381/9626
Type: Thesis
Level: Doctoral
Qualification: PhD
Rights: © The Author, 2011.
Appears in Collections:Theses, Dept. of Physics and Astronomy
Leicester Theses

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