Description
3D models of white dwarf collisions are used to assess the likelihood of double-degenerate mergers as progenitors for Type Ia supernovae (henceforth SNIa) and to identify observational signatures of double-degenerate collisions.
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Contributors
- Hawley, Wendy Phyllis (Author)
- Timmes, Frank (Thesis advisor)
- Young, Patrick (Committee member)
- Starrfield, Sumner (Committee member)
- Fouch, Matt (Committee member)
- Patience, Jennifer (Committee member)
- Arizona State University (Publisher)
Date Created
The date the item was original created (prior to any relationship with the ASU Digital Repositories.)
2012
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Note
- Partial requirement for: Ph.D., Arizona State University, 2012Note typethesis
- Includes bibliographical references (p. 74-78)Note typebibliography
- Field of study: Astrophysics
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by Wendy Phyllis Hawley