Abstract
We present new results from follow-up time-resolved spectroscopy of radial velocity variable hot subdwarfs from the SPY project. Medium resolu- tion spectra were taken at the ESO NTT. Preliminary orbital solutions are presented for three single-lined sdO/B binaries. The orbital periods of all binaries are short and the companions are most likely white dwarfs or late main-sequence stars. Follow-up time-resolved spectroscopy is necessary to measure the orbital parameters with higher accuracy. Light curves should be taken in order to search for reflection effects and or eclipses.
Original language | English |
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Title of host publication | In: Hot Subdwarf Stars and Related Objects - ASP Conf Series 392 |
Publisher | Astronomical Society of the Pacific |
Pages | 225-230 |
ISBN (Print) | 978-1-58381-654-7, 978-1-58381-655-4 |
Publication status | Published - 2008 |