In self-gravitating discs with dust evolution, gravitational-instability and streaming-instability planet-forming regions have different C/O ratio ranges, and total C/O anticorrelates with dust-to-gas ratio.
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C/O ratios in self-gravitating protoplanetary discs with dust evolution
In self-gravitating discs with dust evolution, gravitational-instability and streaming-instability planet-forming regions have different C/O ratio ranges, and total C/O anticorrelates with dust-to-gas ratio.