Post common envelope binaries from SDSS. VIII (Schreiber+, 2010)
The file rv.dat contains the name of the WDMS binary, the time of the spectroscopic observation and the corresponding radial velocity. Using a spectral...
Common envelope events have been associated with the formation of a planetary nebulae since its proposition more than forty five years ago. However, until...
At least 20% of PNe host a post-common-envelope central star, and theoretical considerations predict that a significant fraction of these should come from...
Potential of Photometric Searches for Transiting Planets
Many ground-based photometric surveys are now under way, and five of them have been successful at detecting transiting exoplanets. Nevertheless, detecting...
Power spectra comparison between GOLF and MDI velocity observations
We present a comparison of the velocity power spectra between the GOLF and MDI instruments. In addition, this poster outlines work towards creating a GOLF...