The R136 star cluster dissected with Hubble Space Telescope/STIS - II. Physical properties of the most massive stars in R136

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SEEK ID: https://publications.h-its.org/publications/1180

DOI: 10.1093/mnras/staa2801

Research Groups: Stellar Evolution Theory

Publication type: Journal

Journal: Monthly Notices of the Royal Astronomical Society

Citation: Monthly Notices of the Royal Astronomical Society 499(2):1918-1936

Date Published: 1st Dec 2020

Registered Mode: imported from a bibtex file

Authors: Joachim M. Bestenlehner, Paul A. Crowther, Saida M. Caballero-Nieves, Fabian R. N. Schneider, Sergio Simón-Dı́az, Sarah A. Brands, Alex de Koter, Götz Gräfener, Artemio Herrero, Norbert Langer, Daniel J. Lennon, Jesus Maı́z Apellániz, Joachim Puls, Jorick S. Vink

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Bestenlehner, J. M., Crowther, P. A., Caballero-Nieves, S. M., Schneider, F. R. N., Simón-Díaz, S., Brands, S. A., de Koter, A., Gräfener, G., Herrero, A., Langer, N., Lennon, D. J., Maíz Apellániz, J., Puls, J., & Vink, J. S. (2020). The R136 star cluster dissected with Hubble Space Telescope/STIS – II. Physical properties of the most massive stars in R136. In Monthly Notices of the Royal Astronomical Society (Vol. 499, Issue 2, pp. 1918–1936). Oxford University Press (OUP). https://doi.org/10.1093/mnras/staa2801
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Created: 10th Feb 2021 at 09:59

Last updated: 5th Mar 2024 at 21:24

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