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

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

MESA inlists associated with Aerts et al. (2018). MESA version 10108. Publication DOI: 10.3847/1538-4365/aaccfb

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Bibliographische Detailangaben
Hauptverfasser: Aerts, C., Molenberghs, G., Michielsen, M., Pedersen, M. G., Björklund, R., Johnston, C., Mombarg, J. S. G., Bowman, D. M., Buysschaert, B., Pápics, P. I., Sekaran, S., Sundqvist, J. O., Tkachenko, A., Truyaert, K., Van Reeth, T., Vermeyen, E.
Format: Dataset
Sprache:eng
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Zusammenfassung:MESA inlists associated with Aerts et al. (2018). MESA version 10108. Publication DOI: 10.3847/1538-4365/aaccfb
DOI:10.5281/zenodo.2591743