Hot DA white dwarf model atmosphere calculations: including improved Ni PI cross-sections
To calculate realistic models of objects with Ni in their atmospheres, accurate atomic data for the relevant ionization stages need to be included in model atmosphere calculations. In the context of white dwarf stars, we investigate the effect of changing the Ni IV-VI bound-bound and bound-free atom...
| Main Authors: | , , , , |
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| Other Authors: | |
| Language: | en |
| Published: |
OXFORD UNIV PRESS
2017
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| Subjects: | |
| Online Access: | http://hdl.handle.net/10150/623044 http://arizona.openrepository.com/arizona/handle/10150/623044 |