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Ash, Timothy David Curtis
(1999).
DOI: https://doi.org/10.21954/ou.ro.0000ff7b
Abstract
This thesis deals with observations, and subsequent analysis made of the high-mass X-ray binary systems Cen X-3 and Vela X-l. By making precise radial velocity measurements of the supergiant components, and combining these results with previous X-ray data, the masses of the neutron star components can be determined. The mass of the neutron star in Cen X-3 is found to be 1.21±0.21Mo, while the mass of the neutron star in Vela X-l is found to be 1.77+0.55-0.29Mⵙ. The thesis concludes with an account of an attempt to detect radio emission from the Vela X-l bowshock.
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About
- Item ORO ID
- 65403
- Item Type
- PhD Thesis
- Academic Unit or School
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Faculty of Science, Technology, Engineering and Mathematics (STEM)
Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences - Copyright Holders
- © 1999 Timothy David Curtis Ash
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- ORO Import