Abstract
We present first results from Monte Carlo simulations of short-period sdB plus white dwarf binaries, with various possible distributions of orbital separation and secondary mass. We compare these results with our observed distributions and discuss the implications for the common envelope evolution.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 183-186 |
| Number of pages | 4 |
| Journal | Baltic Astronomy |
| Volume | 15 |
| Issue number | 2 |
| State | Published - 2006 |
Keywords
- Binaries: close
- Methods: numerical
- Stars: hot subdwarfs
- White dwarfs
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science