Table 1: Basic data of the studied Herbig Ae/Be and Vega-like stars.

HD		 Other V Sp. type $\log T_{\rm eff}$ $\log g$ $v\sin{i}$ E(V-L) P [%] Age [Myr] Ref.

Herbig Ae/Be stars

31648		 MWC 480 7.7 A3pesh 3.90-3.95 3.5 102 2 $\hbox{$.\!\!^{\rm m}$ }{}61$ $\sim$0.3 2.5-6 1, 2, 3
38238 V351 Ori 8.9 A7IIIe 3.87-3.89 3.6-3.68 $\sim$100 $2^{\rm m}$-$4^{\rm m}$ - 1-3 4, 5, 6, 7, 8
139614 CD-27 10778 8.2 A7Ve 3.88-3.92 4.0-4.5 13 2 $\hbox{$.\!\!^{\rm m}$ }{}0$ 0.15 5-10 6, 9, 10
144432 CD-42 10650 8.2 A9Ve 3.86-3.87 3.9-4.3 54 1 $\hbox{$.\!\!^{\rm m}$ }{}94$ 0.1-0.5 1-3 2, 9, 10, 11, 12
144668 V856 Sco 7.0 A7IVe 3.89 3.5-4.0 204 $3^{\rm m}$- $3\hbox{$.\!\!^{\rm m}$ }{}5$ 0.5-1.3 0.5-1 2, 3, 6, 10
163296 MWC 275 6.9 A1Ve 3.97 4.0 133 2 $\hbox{$.\!\!^{\rm m}$ }{}96$ 0.5-1.3 3-5 1, 2, 3, 6, 10, 13
190073 MWC 325 7.8 A2IIIe 3.95 3.5 15 2 $\hbox{$.\!\!^{\rm m}$ }{}46$ 0.4 3-5 1, 6, 14

Vega-like stars

26676		 HR 1307 6.2 B8Vn 4.06-4.08 4.0 175 $\sim$ $0\hbox{$.\!\!^{\rm m}$ }$1 0.59 $\sim$70 15, 16
39060 $\beta$ Pic 3.9 A5V 3.91-3.96 4.35 130 0 $\hbox{$.\!\!^{\rm m}$ }{}01$ $\sim$0.02 20-280 17, 18, 19, 20
61712 CD-43 3425 9.0 B7/B8V - - - $\sim$ $0\hbox{$.\!\!^{\rm m}$ }$2 - -  
102647 $\beta$ Leo 2.1 A3V 3.92-3.96 4.30 128 -0 $\hbox{$.\!\!^{\rm m}$ }{}03$ $\sim$0.03 15-330 17, 19, 20, 22
109085 $\eta$ Crv 4.3 F2V 3.83-3.84 4.26 92 -0 $\hbox{$.\!\!^{\rm m}$ }{}13$ $\sim$0.05 950-1560 11, 23, 24, 25
115892 $\iota$ Cen 2.7 A2V 3.96-3.97 - 90 -0 $\hbox{$.\!\!^{\rm m}$ }{}14$ $\sim$0.01 $\sim$500 25
219571 $\gamma$ Tuc 4.0 F1III 3.82-3.88 3.87-3.89 90 0 $\hbox{$.\!\!^{\rm m}$ }{}04$ 0.005 1700-5720 11, 23, 24, 25
[1] Pogodin et al. (2005), [2] Acke & van den Ancker (2004), [3] Natta et al. (1997), [4] Kovalchuk & Pugach (1997), [5] Hernandez et al. (2005), [6] van den Ancker et al. (1998), [7] Marconi et al. (2000), [8] Balona et al. (2002), [9] Dunkin et al. (1997), [10] Sartori et al. (2003), [11] Nordstroem et al. (2004), [12] Pérez et al. (2004), [13] Swartz et al. (2005), [14] Corporon & Lagrange (1999), [15] Stickland (1979), [16] Voshchinnikov & Marchenko (1982), [17] Song et al. (2001), [18] Sheret et al. (2004), [19] Lachaume et al. (1999), [20] Habing et al. (2001), [21] Holmes et al. (2003), [22] Metchev et al. (2004), [23] Ibukiyama & Arimito (2002), [24] Marsakov & Shevelev (1995), [25] Wyatt et al. (2005), [26] Greaves & Wyatt (2003), [27] Lambert & Reddy (2004).


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