Hydrodynamical simulations and similarity relations for eruptive mass-loss from massive stars

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SEEK ID: https://publications.h-its.org/publications/1059

SEEK ID: https://publications.h-its.org/publications/1059

DOI: 10.1093/mnras/stz461

Research Groups: Physics of Stellar Objects, Stellar Evolution Theory

Publication type: Journal

Journal: \mnras

Citation: Monthly Notices of the Royal Astronomical Society 485(1):988-1000

Date Published: 1st May 2019

Registered Mode: imported from a bibtex file

Authors: Stanley P Owocki, Ryosuke Hirai, Philipp Podsiadlowski, Fabian R N Schneider

Citation
Owocki, S. P., Hirai, R., Podsiadlowski, P., & Schneider, F. R. N. (2019). Hydrodynamical simulations and similarity relations for eruptive mass-loss from massive stars. In Monthly Notices of the Royal Astronomical Society (Vol. 485, Issue 1, pp. 988–1000). Oxford University Press (OUP). https://doi.org/10.1093/mnras/stz461
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Created: 17th Feb 2020 at 15:35

Last updated: 5th Mar 2024 at 21:24

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