Table 8: Results of neutron exposures. Columns 2 and 3 correspond to results of the fittings to the theoretical predictions of Malaney (1987a) and Cols. 4 to 7 to those of Malaney (1987b). $S\sp 2$(u), $S\sp 2$(e8), $S\sp 2$(e12) are the fit quality, respectively, for single exposure, exponential exposure under neutron density 10$\sp 8$ cm$\sp {-3}$, and exponential exposure under neutron density 10$\sp {12}$ cm$\sp {-3}$. $\tau _{\rm o}^{\rm a}$, $\tau _{\rm o}^{\rm b}$, and $\tau _{\rm o}^{\rm c}$ are the mean distributions of neutron exposure corresponding to $S\sp 2$(u), $S\sp 2$(e8), and $S\sp 2$(e12), respectively. $\tau _{\rm o}$(f) and $n\sb {\rm n}$ are results corresponding to smaller $S\sp 2$. Column 10 shows if the best fit corresponds to exponential (exp) or single (sing) exposure. Columns 11 to 13 correspond to the results of the fit of $\sigma N$ curves, with $\chi _{\rm red}$ as the quality of the fit. Numbers in parenthesis are errors in last decimals and were estimated directly from the fittings. The uncertainties on $\tau _{\rm o}^{\rm a}$, $\tau _{\rm o}^{\rm b}$, and  $\tau _{\rm o}^{\rm c}$ were estimated in 0.1 mb$\sp {-1}$. For all cases, $\tau _{\rm o}$ is given in mb$\sp {-1}$.

Star		 S2(u) $\tau _{\rm o}^{\rm a}$ S2(e8) $\tau _{\rm o}^{\rm b}$ S2(e12) $\tau_{\rm o}^c$ $\tau _{\rm o}$(f) $n_{\rm n}$ exp $\tau _{\rm o}$($\sigma N$) G(%) $\chi _{\rm red}$

HD 749		 0.69 1.00 0.52 0.80 0.77 0.80 0.8 108 exp 0.406(5) 0.568(19) 0.73
HR 107 0.98 0.10 1.47 0.20 1.30 0.30 0.1 108 sing 0.43(6) 0.083(20) 0.56
HD 5424 0.85 1.10 1.15 0.80 1.71 0.80 1.1 108 sing 1.05(1) 0.086(1) 0.94
HD 8270 1.33 0.90 1.21 0.20 1.46 0.30 0.2 108 exp 0.27(1) 0.35(3) 0.41
HD 12392 0.46 1.10 0.38 0.80 0.79 0.80 0.8 108 exp 0.40(2) 0.73(3) 0.59
HD 13551 1.57 0.90 1.25 0.20 1.44 0.30 0.2 108 exp 0.22(1) 1.06(56) 0.50
HD 22589 1.10 0.80 0.89 0.20 1.27 0.20 0.2 108 exp 0.187(23) 1.25(54) 0.52
HD 27271 0.26 0.90 0.24 0.40 0.16 0.05 0.05 1012 exp 0.272(14) 0.568(19) 0.35
HD 48565 3.14 1.00 1.34 0.40 2.66 0.05 0.4 108 exp 0.659(10) 0.0631(23) 0.32
HD 76225 0.80 0.10 0.71 0.20 1.83 0.30 0.2 108 exp 0.25(1) 0.83(12) 0.38
HD 87080 2.22 1.00 1.17 0.60 2.49 0.80 0.6 108 exp 0.71(1) 0.145(5) 0.48
HD 89948 0.67 0.10 0.45 0.20 1.65 0.30 0.2 108 exp 0.24(2) 0.77(36) 0.30
HD 92545 1.42 0.90 1.22 0.20 0.85 0.30 0.3 1012 exp 0.291(3) 0.261(14) 0.40
HD 106191 1.36 0.90 1.16 0.40 0.72 0.05 0.05 1012 exp 0.383(1) 0.130(1) 0.38
HD 107574 1.91 0.90 2.28 0.20 2.05 0.30 0.9 108 sing 0.298(2) 0.245(5) 0.42
HD 116869 0.14 1.10 0.18 0.80 0.33 0.80 1.1 108 sing 0.55(2) 0.0646(22) 0.55
HD 123396 0.46 1.10 0.84 0.80 1.24 0.80 1.1 108 sing 0.54(2) 0.0315(22) 0.54
HD 123585 2.17 1.00 0.98 0.40 2.14 0.50 0.4 108 exp 0.46(1) 0.275(15) 0.46
HD 147609 2.33 0.10 1.90 0.20 2.42 0.30 0.2 108 exp 0.288(7) 1.07(11) 0.41
HD 150862 0.66 0.90 1.57 0.20 1.11 0.30 0.9 108 sing 0.271(3) 0.489(26) 0.47
HD 188985 1.83 0.90 1.77 0.40 1.94 0.40 0.4 108 exp 0.401(4) 0.225(5) 0.39
HD 210709 0.11 1.10 0.19 0.80 0.26 0.80 1.1 108 sing 0.314(3) 0.303(9) 0.38
HD 210910 0.55 0.10 0.63 0.20 0.38 0.30 0.3 1012 exp 0.44(4) 0.075(13) 0.52
HD 222349 3.02 0.90 1.28 0.40 2.00 0.05 0.4 108 exp 0.379(8) 0.170(12) 0.46
BD+18 5215 2.41 0.90 2.74 0.40 1.50 0.05 0.05 1012 exp 0.274(1) 0.503(2) 0.63
HD 223938 0.26 1.00 0.20 0.50 0.29 0.70 0.5 108 exp 0.384(5) 0.229(9) 0.34


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