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The collapse of rotating stellar cores: the amount of gravitational radiation predicted by various numerical models

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Müller,  E.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Müller, E. (1984). The collapse of rotating stellar cores: the amount of gravitational radiation predicted by various numerical models. In D. Bancel, & M. Signore (Eds.), Problems of Collapse and Numerical Relativity (pp. 271-286). Dordrecht, The Netherlands: Reidel Publishing Company.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0011-BD98-3
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