Morphology and Mach Number Dependence of Subsonic Bondi–Hoyle Accretion

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SEEK ID: https://publications.h-its.org/publications/1852

SEEK ID: https://publications.h-its.org/publications/1852

DOI: 10.3847/1538-4357/ad3732

Research Groups: Physics of Stellar Objects

Publication type: Journal

Journal: \apj

Citation: ApJ 966(1):103

Date Published: 29th Apr 2024

Registered Mode: imported from a bibtex file

Authors: Logan J. Prust, Hila Glanz, Lars Bildsten, Hagai B. Perets, Friedrich K. Röpke

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Prust, L. J., Glanz, H., Bildsten, L., Perets, H. B., & Röpke, F. K. (2024). Morphology and Mach Number Dependence of Subsonic Bondi–Hoyle Accretion. In The Astrophysical Journal (Vol. 966, Issue 1, p. 103). American Astronomical Society. https://doi.org/10.3847/1538-4357/ad3732
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Created: 19th Jul 2024 at 11:46

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