Formation of short-period planets by disc migration
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DOI: 10.1093/mnras/stz974
Abstract: Protoplanetary discs are thought to be truncated at orbital periods of around 10 d. Therefore, the origin of rocky short-period planets with P < 10 d is a puzzle. We propose that many of these planets may… read more here.
Keywords: short period; formation short; period; period planets ... See more keywords