Cambridge University Press, Proceedings of the International Astronomical Union, S253(4), p. 420-423, 2008
DOI: 10.1017/s1743921308026823
Full text: Unavailable
AbstractWe present an analysis of the HD planetary system based on a photometric transit dataset and radial velocities obtained on 3 December 2007. We also present limits on the presence of close stellar companions based on high resolution images.