A flat inner disc model as an alternative to the Kepler dichotomy in the Q1-Q16 planet population

T. Bovaird*, T. Bovaird*, C. H. Lineweaver*, C. H. Lineweaver*, C. H. Lineweaver*

*Corresponding author for this work

    Research output: Contribution to journal › Article › peer-review

    11 Citations (Scopus)

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    Physics