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Table 2:

Targets discussed in this paper.
Object $v\sin i$ log M $_{\rm acc}$ IR Comp. log $T_{\rm eff}$ log L M Age
name [km s-1] [$M_{\odot}$/yr] feature   [K] [$L_{\odot}$] [$M_{\odot}$] [Myr]
PDS 2 175a     no 3.98d 1.68d 2.5  
HD 47839* 120b     yesee 4.57uu 5.23uu   $\sim $0.3eee
HD 95881 50c -8.04 Si, PAHr yesff 3.86vv 1.84vv 3.1 >3x
HD 97048 140d -7.17 PAHs nogg 4.00s 1.64s 2.5 >2d
HD 97300   <-8.18 PAHt yeshh 4.02ww 1.54ww 2.5 >3ww
HD 100453 39e -8.04 PAHu yesii 3.87s 0.90s 1.7 $14\pm4$x
HD 100546 65f   Si, PAHu nogg 4.02s 1.51s 2.5 >10d
HD 101412 5g   Si, PAHv yesgg 3.98xx 1.74xx 2.5 $\sim $2fff
HD 135344B 69h -8.27 Sis, PAHw yesjj 3.82s 0.91s 1.6 $8\pm 4^{x}$
HD 139614 15i -7.99 Siu yesee 3.90s 0.91s 1.8 >10x
HD 144432 70i -7.07 Siu yeskk 3.87s 1.01s 1.8 $10\pm 5^{x}$
HD 144668 100i -6.37 Six yesll 3.90s 1.94s 3.1 $0.6\pm 0.4^{ww}$
HD 150193 100f -7.29 Sis yesmm 3.95s 1.38s 2.2 >2d
HD 152404 18.5j   Siy yesj 3.81s 0.95s 1.7 $\sim $8vv
HD 158643 267h/228k -6.87 Siu nonn 4.00d 2.39d 3.9 0.3d
HD 163296 130i -7.12 Siu nogg 3.94s 1.38s 2.2 $5\pm2$x
HD 169142 66h -7.40 PAHw yesoo 3.91s 1.16s 2.0 $6\pm3$x
VV Ser 142a/229l -6.34 Siz nogg 3.95s 1.27s 2.0 $3.5\pm0.5$ggg
HD 176386   -8.11 PAHaa yesee 4.03ww 1.69ww 2.7 >2ww
HD 179218 60b -6.59 Si, PAHu nogg 4.02s 2.00s 3.0 $1.3\pm0.5$x
HD 190073 12i   Si, PAHr yesff 3.95d 1.80d 2.7 $1.2\pm0.6$hhh
Stars with debris disks
HD 9672 196k   -bb no 4.00yy 1.42yy 2.3 $\sim $8iii
HD 39060 130m   Sicc no 3.91zz 0.95zz 1.8 $\sim $12jjj
HD 109573 152k <-8.53 -bb yespp 3.97aaa 1.32aaa 2.2 $\pm$ 2pp
HD 164249       yesqq 3.81bbb 0.48n 1.4 $\sim $12jjj
HD 172555     Sidd no 3.89bbb 0.96n 1.7 $\sim $12jjj
HD 181327 16n     no 3.81bbb 0.54n 1.4 $\sim $12jjj
Magnetic Herbig Ae/Be stars from previous studies
HD 31648* 90o   Sis norr 3.94s 1.14s 2.0 $\sim $7kkk
HD 104237* 10h -7.45 Sis yesss 3.93s 1.54s 2.2 $2.0\pm0.5$ww
HD 200775* 26p     yestt 4.29s 3.82s   $0.1\pm0.05$ww
V380 Ori 200f   Six yesee 3.97d 2.04ddd 3.0 $1.5\pm0.5$x
BF Ori 37l   Sis no 3.95s 1.53s 2.3 $\sim $2lll
Standard Ap star with a weak magnetic field
HD 162725 32q       3.99ccc 2.33ccc    
Notes: The information on $v\sin i$ values, mass-accretion rate, IR features, binarity, effective temperature, luminosity, and age was collected from the literature. The mass was deduced from the position of the star in the H-R diagram (see Sect. 5). Objects marked with * are excluded from the correlation analysis (see Sects. 2, 4.3, and 5.1).
References: a Vieira et al. (2003), b Bernacca & Perinotto (1970), c Grady et al. (1996), d van den Ancker et al. (1998), e Acke & Waelkens (2004), f Hamidouche et al. (2008), g this work, h Dunkin et al. (1997), i Hubrig et al. (2007b), j Alencar et al. (2003), k Royer et al. (2007), l Mora et al. (2001), m Slettebak (1982), n de la Reza & Pinzón (2004), o Beskrovnaya et al. (2004), p Alecian et al. (2008), q Landstreet et al. (2008), r Boersma et al. (2008), s Acke & van den Ancker (2004), t Siebenmorgen et al. (1998), u Meeus et al. (2001), v Geers et al. (2007), w Sloan et al. (2005), x van Boekel et al. (2005), y Przygodda et al. (2003), z Pontoppidan et al. (2007b), aa Siebenmorgen et al. (2000), bb Kessler-Silacci et al. (2005), cc Okamoto et al. (2004), dd Schütz et al. (2005b), ee Dommanget & Nys (1994), ff Baines et al. (2006), gg Corporon & Lagrange (1999), hhStelzer et al. (2006), ii Chen et al. (2006a), jj Augereau et al. (2001), kk Carmona et al. (2007), ll Stecklum et al. (1995), mm Reipurth & Zinnecker (1993), nn Roberge et al. (2002), oo Grady et al. (2007), pp Stauffer et al. (1995), qq SIMBAD, rr Eisner et al. (2004), ss Grady et al. (2004), tt Pirzkal et al. (1997), uu Schnerr et al. (2007), vv Blondel et al. (2006), ww van den Ancker et al. (1997), xx Wade et al. (2007), yy Hughes et al. (2008), zz di Folco et al. (2004), aaa Debes et al. (2008), bbb Zuckerman & Song (2004), ccc Folsom et al. (2007), ddd Corcoran & Ray (1998), eee Walsh (1980), fff Wade et al. (2005), ggg Pontoppidan et al. (2007a), hhh Catala et al. (2007), iii Thi et al. (2001), jjj Zuckerman et al. (2001), kkk Simon et al. (2000), and lll Natta et al. (1997).

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