On the possibility that the most massive stars result from binary mergers

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SEEK ID: https://publications.h-its.org/publications/1984

DOI: 10.1051/eas/1364003

Research Groups: Stellar Evolution Theory

Publication type: InProceedings

Journal: EAS Publications Series

Book Title: EAS Publications Series

Editors: Pavlovski, K. and Tkachenko, A. and Torres, G.

Citation: EAS Publications Series 64:21-28

Date Published: 2013

Registered Mode: imported from a bibtex file

Authors: A. de Koter, J. M. Bestenlehner, S. E. de Mink, C. J. Evans, G. Gräfener, R. G. Izzard, N. Langer, O. H. Ramı́rez-Agudelo, H. Sana, F. R. N. Schneider, S. Simón-Dı́az, J. S. Vink

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Fabian Schneider

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de Koter, A., Bestenlehner, J. M., de Mink, S. E., Evans, C. J., Gräfener, G., Izzard, R. G., Langer, N., Ramírez-Agudelo, O. H., Sana, H., Schneider, F. R. N., Simón-Díaz, S., & Vink, J. S. (2013). On the possibility that the most massive stars result from binary mergers. In K. Pavlovski, A. Tkachenko, & G. Torres (Eds.), EAS Publications Series (Vol. 64, pp. 21–28). EDP Sciences. https://doi.org/10.1051/eas/1364003

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Created: 21st Jan 2025 at 20:41

On the possibility that the most massive stars result from binary mergers

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