Table 7: Photometric solutions for AD Boo (all data) from the WD code adopting linear limb darkening coefficients by van Hamme (1993); see Table 6. Gravity darkening exponents of 0.33 and bolometric albedo coefficients of 0.5 were applied, as appropriate for convective envelopes. $T_{\rm {eff},p}$ was assumed to be 6575 K.
  y b v u
i   ($^\circ$) 87.47 87.78 87.79 87.82
  $\pm$5 $\pm$3 $\pm$3 $\pm$6

$\Omega_{\rm p}$

 6.743 6.711 6.717 6.702
  $\pm$11 $\pm$8 $\pm$9 $\pm$14

$\Omega_{\rm s}$

 7.646 7.696 7.675 7.636
  $\pm$16 $\pm$10 $\pm$9 $\pm$18

$r_{\rm p}$

 0.1705 0.1713 0.1711 0.1716

$r_{\rm s}$

 0.1303 0.1293 0.1297 0.1305

k

 0.764 0.755 0.758 0.761

$r_{\rm p} + r_{\rm s}$

 0.3008 0.3006 0.3008 0.3021

$T_{\rm {eff},s}$

 6078 6052 5999 5946
  $\pm$4 $\pm$4 $\pm$4 $\pm$4

$L_{\rm s}/L_{\rm p}$

 0.4205 0.3868 0.3615 0.3761

$\sigma$   (mag.)

 0.0064 0.0062 0.0066 0.0101


Source LaTeX | All tables | In the text