Description
I examine the effects of metallicity on solar mass stellar evolution, trying to replicate a previous result in Windhorst et.al., 2018, in which a zer metallicity solar mass star did not reach the AGB, and thus may turn into a helium white dwarf. In trying to replicate this result, I used the M.E.S.A. stellar evolution code and was unable to reproduce this result.
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Contributors
- Tompkins, Scott Andrew (Author)
- Windhorst, Rogier (Thesis director)
- Young, Patrick (Committee member)
- School of Earth and Space Exploration (Contributor)
- Department of Physics (Contributor)
- Barrett, The Honors College (Contributor)
Date Created
The date the item was original created (prior to any relationship with the ASU Digital Repositories.)
2019-12
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