The role of supernova convection for the lower mass gap in the isolated binary formation of gravitational wave sources

ABSTRACT Understanding the astrophysical phenomena involving compact objects requires an insight about the engine behind the core-collapse supernovae (SNe) and the fate of the stellar collapse of massive stars. In particular, this insight is crucial in developing an understanding of the origin and f...

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Bibliographic Details
Published in:Monthly notices of the Royal Astronomical Society 2022-09, Vol.516 (2), p.2252-2271
Main Authors: Olejak, Aleksandra, Fryer, Chris L, Belczynski, Krzysztof, Baibhav, Vishal
Format: Article
Language:English
Subjects:
ASTRONOMY AND ASTROPHYSICS
binary stars
black hole - neutron star mergers
black hole mergers
black holes
gravitational waves
neutron star mergers
Physical data and processes
stars
supernovae
transients
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