SIMBAD references

2013MNRAS.435.2328D - Mon. Not. R. Astron. Soc., 435, 2328-2334 (2013/November-1)

The curiously circular orbit of Kepler-16b.

DUNHILL A.C. and ALEXANDER R.D.

Abstract (from CDS):

The recent discovery of a number of circumbinary planets lends a new tool to astrophysicists seeking to understand how and where planet formation takes place. Of the increasingly numerous circumbinary systems, Kepler-16 is arguably the most dynamically interesting: it consists of a planet on an almost perfectly circular orbit (e = 0.0069) around a moderately eccentric binary (e = 0.16). We present high-resolution 3D smoothed particle hydrodynamics simulations of a Kepler-16 analogue embedded in a circumbinary disc, and show that the planet's eccentricity is damped by its interaction with the protoplanetary disc. We use this to place a lower limit on the gas surface density in the real disc through which Kepler-16b migrated of Σmin ∼ 10g/cm2. This suggests that Kepler-16b, and other circumbinary planets, formed and migrated in relatively massive discs. We argue that secular evolution of circumbinary discs requires that these planets likely formed early on in the lifetime of the disc and migrated inwards before the disc lost a significant amount of its original mass.

Abstract Copyright: © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2013)

Journal keyword(s): hydrodynamics - planets and satellites: dynamical evolution and stability - planets and satellites: individual: Kepler-16b - planet-disc interactions - protoplanetary discs - binaries: close

Simbad objects: 10

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2013MNRAS.435.2328D and select 'bookmark this link' or equivalent in the popup menu


2019.12.09-12:05:17

© Université de Strasbourg/CNRS

    • Contact