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Table 5:

Astrophysical properties of 31 Comae.

Parameter
Value Based on
V0, mag 4 $.\!\!^{\rm m}$935 APT V photometry
Distance, pc 89.1 +1.9-1.7 revised Hipparcos
MV $+0\hbox{$.\!\!^{\rm m}$ }19\pm0.05$ from V0 and distance
Classification, MK G0III Gray et al. (2001a)
Temperature, K 5810 Gray et al. (2001a)
  $5660 \pm 42$ STELLA spectra
Radius, $R_\odot$ $8.74 \pm 1.1$ angular diameter
Minimum radius, $R_\odot$ $8.95 \pm 0.27$ from $P_{\rm rot}$ & $v \sin i$
Luminosity, $L_\odot$ $73.2 \pm 4$ from MV and B.C.
  $77.7 \pm 13$ from R and $T_{\rm eff}$
Gravity, cgs 3.42 Gray et al. (2001a)
  $3.51 \pm 0.09$ STELLA spectra
Mass, $M_\odot$ $2.6 \pm 0.1$ evolutionary tracks
Age, Myr 540+24-21 isochrone fitting
Metallicity, [M/H] -0.21 Gray et al. (2001a)
  -0.17 GC, Strömgren phot.
  - $0.15\pm0.03$ STELLA spectra
Li abundance, H=12 $3.0 \pm 0.15$ STELLA spectra
Average RV, km s-1 +$0.10\pm$0.33 STELLA spectra
$v \sin i$, km s-1 $67 \pm 2$ STELLA spectra
Rotation period, days $6.80 \pm 0.06$ MOST photometry
  $7.04 \pm 0.12$ APT y photometry
  $6.76 \pm 0.02$ STELLA radial velocity
Inclination, deg $\approx $80 adopted

Notes. Values not cited in the third column were obtained in this paper. GC=Geneva-Copenhagen survey.


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