Figure 1
The solid line indicates the best-fitting single Keplerian which has an rms of 6.6 m sā1 fit to the data. The Keck data are shown as squares and the AAT data as circles.
The solid line indicates the best-fitting single Keplerian which has an rms of 6.6 m sā1 fit to the data. The Keck data are shown as squares and the AAT data as circles.
