Forward Asteroseismic Modeling of Stars with a Convective Core from Gravity-mode Oscillations: Parameter Estimation and Stellar Model Selection-Reference-Cited by-同舟云学术

Forward Asteroseismic Modeling of Stars with a Convective Core from Gravity-mode Oscillations: Parameter Estimation and Stellar Model Selection

Published:2018-07-19 Issue:1 Volume:237 Page:15
ISSN:1538-4365
Container-title:The Astrophysical Journal Supplement Series
language:
Short-container-title:ApJS

Author:

Aerts C.^ORCID,Molenberghs G.,Michielsen M.,Pedersen M. G.,Björklund R.,Johnston C.,Mombarg J. S. G.,Bowman D. M.,Buysschaert B.,Pápics P. I.^ORCID,Sekaran S.,Sundqvist J. O.,Tkachenko A.,Truyaert K.,Reeth T. Van,Vermeyen E.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4365/aaccfb/pdf

Reference173 articles.

1. Asteroseismology

2. Discovery of the New Slowly Pulsating B Star HD 163830 (B5 II/III) from MOST Space-based Photometry

3. THE SURFACE NITROGEN ABUNDANCE OF A MASSIVE STAR IN RELATION TO ITS OSCILLATIONS, ROTATION, AND MAGNETIC FIELD

4. Asteroseismology of HD 129929: Core Overshooting and Nonrigid Rotation

5. The Interior Angular Momentum of Core Hydrogen Burning Stars from Gravity-mode Oscillations

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