Collective velocity broadening from gravity waves as a plausible mechanism for macroturbulence in massive stars

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SEEK ID: https://publications.h-its.org/publications/1428

SEEK ID: https://publications.h-its.org/publications/1428

DOI: 10.5281/zenodo.5525398

Research Groups: Physics of Stellar Objects

Publication type: InProceedings

Book Title: MOBSTER-1 virtual conference: Stellar Variability as a Probe of Magnetic Fields in Massive Stars

Citation: In MOBSTER-1 virtual conference: Stellar Variability as a Probe of Magnetic Fields in Massive Stars, p. 15

Date Published: 1st Sep 2021

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Registered Mode: imported from a bibtex file

Authors: D. M. Bowman, S. Burssens, S. Simón-Dı́az, P. V. F. Edelmann, T. M. Rogers, L. Horst, F. K. Röpke, C. Aerts

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Bowman, D. M., Burssens, S., Simón-Díaz, S., Edelmann, P. V. F., Rogers, T. M., Horst, L., Röpke, F. K., & Aerts, C. (2021). Collective velocity broadening from gravity waves as a plausible mechanism for macroturbulence in massive stars. https://doi.org/10.5281/ZENODO.5525398
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Created: 20th Dec 2021 at 16:33

Last updated: 5th Mar 2024 at 21:24

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