Table 1: Basic data of the studied Herbig Ae stars.
HD Other V Sp. type $T_{\rm eff}$ $\log~G$ $v~\sin i$ Ref. $(V-L)_{\rm obs}$ P $\left<{\cal B}_z\right>$
139614 CD-27 10778 8.2 A7Ve 8250 4.5 13 (1) $\sim$2 $\hbox{$.\!\!^{\rm m}$ }0$ $\sim$0.1-0.5% $-450\pm 93$ G
144432 CD-42 10650 8.2 A9Ve 7750 4.5 54 (1) $\sim$2 $\hbox{$.\!\!^{\rm m}$ }0$ $\sim$0.1-0.5% $-94\pm60$ G
144668 HR 5999 7.0 A7IVe 7800 3.5-4.0 180 (2) $3\hbox{$.\!\!^{\rm m}$ }0$- $3\hbox{$.\!\!^{\rm m}$ }5$ $\sim$0.5-1.3% $-118\pm48$ G

(1) Meeus et al. (1998); (2) Grady et al. (1994).


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