Skip navigation
Skip navigation

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

Bovaird, Timothy; Lineweaver, Charles

Description

We use simulated planetary systems to model the planet multiplicity of Kepler stars. Previous studies have underproduced single planet systems and invoked the so-called Kepler dichotomy, where the planet forming ability of a Kepler star is dichotomous, producing either few or many transiting planets. In this paper, we show that the Kepler dichotomy is only required when the inner part of planetary discs are just assumed to be flared. When the inner part of planetary discs are flat, we reproduce...[Show more]

CollectionsANU Research Publications
Date published: 2017
Type: Journal article
URI: http://hdl.handle.net/1885/197018
Source: Monthly Notices of the Royal Astronomical Society
DOI: 10.1093/mnras/stx414
Access Rights: Open Access

Download

File Description SizeFormat Image
01_Bovaird_A_flat_inner_disc_model_as_an_2017.pdf2.56 MBAdobe PDFThumbnail


Items in Open Research are protected by copyright, with all rights reserved, unless otherwise indicated.

Updated:  19 May 2020/ Responsible Officer:  University Librarian/ Page Contact:  Library Systems & Web Coordinator