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CVs: Short Period Systems
CVs with main sequence secondaries have minimum orbital period of 80 minutes
However, some accreting binaries are seen to have shorter periods
Þ the secondaries must be white dwarfs, or perhaps the
degenerate core of a giant which has been stripped away
The optical spectra of these systems show only Helium (no Hydrogen)
GP Com
The disk behaviour is different because of the different ionisation of He compared to He; interesting astrophysical laboratories
Orbital periods from ~65 min to ~15 min
Known as the AM CVn systems
Marsh, Horne & Rosen (1991)