The Effects of the Carbon-to-oxygen Ratio on the Condensate Compositions around Solar-like Stars
The initial stellar carbon-to-oxygen (C/O) ratio can have a large impact on the resulting condensed species present in the protoplanetary disk and, hence, the composition of the bodies and planets that form. The observed C/Os of stars can vary from 0.1–1. We use a sequential dust condensation model...
| Main Authors: | , , , , |
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| 格式: | 文件 |
| 语言: | English |
| 出版: |
IOP Publishing
2025-01-01
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| 丛编: | The Astronomical Journal |
| 主题: | |
| 在线阅读: | https://doi.org/10.3847/1538-3881/adaead |