Observational evidence of coalescence as a viable cause of magnetism in massive stars

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SEEK ID: https://publications.h-its.org/publications/1310

DOI: 10.5281/zenodo.5042167

Research Groups: Stellar Evolution Theory

Publication type: InProceedings

Book Title: OBA Stars: Variability and Magnetic Fields

Citation: In OBA Stars: Variability and Magnetic Fields, p. 19

Date Published: 1st Jun 2021

Registered Mode: imported from a bibtex file

Authors: A. J. Frost, L. Mahy, H. Sana, R. H. Barba, J. Barron, D. M. Bowman, M. Fabry, J. -B. Le Bouquin, N. I. Morrell, P. Marchant, A. Merand, M. Munoz, F. R. N. Schneider, T. Shenar, G. Wade

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Frost, A. J., Mahy, L., Sana, H., Barba, R. H., Barron, J., Bowman, D. M., Fabry, M., Bouquin, J.-B. L., Morrell, N. I., Marchant, P., Merand, A., Munoz, M., Schneider, F. R. N., Shenar, T., & Wade, G. (2021). Observational evidence of coalescence as a viable cause of magnetism in massive stars. https://doi.org/10.5281/ZENODO.5042167
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Created: 11th Nov 2021 at 22:40

Last updated: 5th Mar 2024 at 21:24

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