Document Type

Article

Publication Date

9-25-2019

Publication Title

Monthly Notices of the Royal Astronomical Society

Publisher

Oxford University Press

Volume

490

Issue

1

First page number:

1332

Last page number:

1349

Abstract

An initially sufficiently misaligned low-mass protoplanetary disc around an eccentric binary undergoes damped nodal oscillations of tilt angle and longitude of ascending node. Dissipation causes evolution towards a stationary state of polar alignment in which the disc lies perpendicular to the binary orbital plane with angular momentum aligned to the eccentricity vector of the binary. We use hydrodynamic simulations and analytical methods to investigate how the mass of the disc affects this process. The simulations suggest that a disc with non-zero mass settles into a stationary state in the frame of the binary, the generalized polar state, at somewhat lower levels of misalignment with respect to the binary orbital plane, in agreement with the analytical model. Provided that discs settle into this generalized polar state, the observational determination of the misalignment angle and binary properties can be used to determine the mass of a circumbinary disc. We apply this constraint to the circumbinary disc in HD 98800. We obtain analytical criteria for polar alignment of a circumbinary ring with mass that approximately agree with the simulation results. Very broad misaligned discs undergo breaking, but the inner regions at least may still evolve to a polar state. The long-term evolution of the disc depends on the evolution of the binary eccentricity that we find tends to decrease. Although the range of parameters required for polar alignment decreases somewhat with increasing disc mass, such alignment appears possible for a broad set of initial conditions expected in protostellar circumbinary discs.

Keywords

Accretion, accretion discs; Hydrodynamics; Planets and satellites: formation; Binaries: general

Disciplines

Stars, Interstellar Medium and the Galaxy

File Format

pdf

File Size

1.834 KB

Language

English

Creative Commons License

Creative Commons Attribution 4.0 License
This work is licensed under a Creative Commons Attribution 4.0 License.

Download

UNLV article access

Search your library

Share

COinS