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Gravity-wave asteroseismology of intermediate- and high-mass stars

Lookup NU author(s): Professor Tamara Rogers, Rathish Ratnasingam

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This is the authors' accepted manuscript of an article that has been published in its final definitive form by AAS Publishing, 2019.

For re-use rights please refer to the publisher's terms and conditions.


Abstract

This white paper focuses specifically on the transport of chemical elements and of angular momentum in the stellar structure and evolution models of stars born with convective core, as revealed by their gravity-mode oscillations.


Publication metadata

Author(s): Tkachenko A, Aerts C, Bowman DM, Van Reeth T, De Ridder J, Johnston CC, Pedersen MG, Burssens S, Michielsen M, Mombarg J, Sekaran S, Bjorklund R, Rogers TM, Edelmann PVF, Ratnasingam RP, Zwintz K, Kollmeier J, Johnson J, Rix HW, Tayar J

Publication type: Article

Publication status: Published

Journal: Bulletin of the American Astronomical Society

Year: 2019

Volume: 51

Issue: 3

Online publication date: 31/05/2019

Acceptance date: 01/05/2019

Date deposited: 08/08/2019

ISSN (print): 0002-7537

ISSN (electronic): 2330-9458

Publisher: AAS Publishing

URL: https://baas.aas.org/wp-content/uploads/2019/05/198_tkachenko.pdf

Notes: Astro2020: Decadal Survey on Astronomy and Astrophysics, science white papers


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