AM CVN stars -an update Jan-Erik Solheim Institute ofTheoreticalPhysics University of Oslo.
Where are the Accreting Helium White Dwarfs?? Drawing by T. Piro.
Asteroseismology of evolved stars: from hot B subdwarfs to white dwarfs
The Empirical Mass Distribution of Hot B Subdwarfs derived by asteroseismology and other means Valerie Van Grootel (1) G. Fontaine (2), P. Brassard (2),
