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Accretion induced collapse of white dwarfs in binary systems and their observational properties

Wickramasinghe, Dayal; Hurley, Jarrod; Ferrario, Lilia; Tout, Christopher A; Kiel, Paul D

Description

Neutron stars can form through core collapse (CC) following a supernova explosion of a massive star, or from a white dwarf that first forms in a binary system and then collapses into a neutron star via accretion induced collapse (AIC). So far, there have

CollectionsANU Research Publications
Date published: 2009
Type: Journal article
URI: http://hdl.handle.net/1885/35814
Source: Journal of Physics: Conference Series
DOI: 10.1088/1742-6596/172/1/012037

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