Slide 1 Binary Star Evolution Half of all stars are in binary systems - stellar evolution in binaries is important Roche Lobe: 3-D boundary where the gravity of 2 stars is…
Asteroseismology of evolved stars: from hot B subdwarfs to white dwarfs Valerie Van Grootel Université de Liège, FNRS Research Associate Main collaborators: AG2014 –…
Cataclysmic Variable Stars Nataliya Ostrova Astronomical observatory of the Odessa National University, [email protected] T.G. Shevchenko Park, Odessa, Ukraine [email protected]…
The Empirical Mass Distribution of Hot B Subdwarfs derived by asteroseismology and other means Valerie Van Grootel(1) G. Fontaine(2), P. Brassard(2), S. Charpinet(3), E.M.…