In 1988, Campbell et al also reported finding
small velocity variations that could be the result of a substellar object of one to nine times the mass of Jupiter that may orbit Xi Boötis B.
Not exact matches
Prior to 2009,
small but significant
variations in radial
velocity had been detected which may have been caused by a substellar companion of one to nine Jupiter - masses with an orbital period of 50 years of less (Campbell et al, 1988, pages 904, 906, and 919).
Kepler - 19 joins the
small number of systems that reconcile transit timing
variation and radial
velocity measurements.
If you are new to this saga make sure you read Tau II Abstract: The successful detection is reported of radial -
velocity variations due to orbital motion of the substellar companion of the star tau Boötis, from data obtained with a
small aperture (0.4 - m) telescope and a fibre - fed high resolution spectrograph.
The detected
velocity variations were too
small to be cause by a body orbiting star A, which is more massive (see HR 5544 on page 919).