K. Fuhrmann et al., F-TYPE AND G-TYPE STARS WITH PLANETARY COMPANIONS - UPSILON-ANDROMEDAE, RHO(1) CANCRI, TAU-BOOTIS, 16-CYGNI AND RHO-CORONAE-BOREALIS, Astronomy and astrophysics (Berlin), 336(3), 1998, pp. 942-952
Accurate stellar parameters are presented for the F- and G-type stars
nu And, rho(1) Cnc, tau Boo, 16 Cyg, and rho CrB, which are deemed to
possess planetary companions from intense Doppler monitoring. Evolutio
nary tracks that employ detailed around wt: model atmospheres as upper
boundary condition and allow for al. (1997). helium diffusion are com
puted for the individual stars to derive the stellar masses and ages.
From a comparison of the spectroscopic parallaxes with the accurate di
stances available from the Hipparcos satellite well-defined constraint
s on the stellar surface gravities are obtained in good agreement with
out spectroscopically deduced values.