The primary shows long -
period radial velocity variations that indicate the presence of a low mass companion whose projected mass is in the planetary regime (m sin i = 9.33 Mjup).
Not exact matches
The
radial -
velocity variations indicate a highly eccentric orbit with a
period of 153.9 days.
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).
As CORVAL monitoring failed to detect significant
radial velocity variations over
period of 3,400 days — or over 9.3 years (Duquennoy and Mayor, 1991, pp. 492 and 506), the detection is now considered to be spurious.
High - precision
radial -
velocity measurements confirm a sinusoidal
variation with the
period and phase predicted by the photometry, and rule out the presence of line - bisector
variations that would indicate that the spectroscopic orbit is spurious.