Abstract
Ultra-compact binaries are objects which have orbital periods shorter than one hour. Both stars
must be compact and are typically degenerate and hydrogen deficient. The class includes interacting
AM CVn stars, ultra-compact X-ray binaries, detached double white dwarfs, double neutron
stars, white dwarf/neutron star binaries and as yet unobserved binaries such as black holes with
neutron star or white dwarf companions.
| Original language | Undefined/Unknown |
|---|---|
| Publisher | Unknown Publisher |
| Publication status | Published - 2009 |
Bibliographical note
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