\begin{table}%t2 \caption {\label{tab:targetvals}Targets discussed in this paper.} %\centerline {\begin{tabular}{lllllllll} \hline \hline \multicolumn{1}{c}{Object \rule{0pt}{2.6ex}} & \multicolumn{1}{c}{$v\sin i$} & \multicolumn{1}{c}{log {\it \. M}$_{\rm acc}$} & \multicolumn{1}{c}{IR } & \multicolumn{1}{c}{Comp.} & \multicolumn{1}{c}{log $T_{\rm eff}$} & \multicolumn{1}{c}{log $L$} & \multicolumn{1}{c}{$M$} & \multicolumn{1}{c}{Age} \\ \multicolumn{1}{c}{name} & \multicolumn{1}{c}{[km~s$^{-1}$]} & \multicolumn{1}{c}{[$M_{\odot}$/yr]} & \multicolumn{1}{c}{feature} & & \multicolumn{1}{c}{[K]} & \multicolumn{1}{c}{[$L_{\odot}$]} & \multicolumn{1}{c}{[$M_{\odot}$]} & \multicolumn{1}{c}{[Myr]} \\ \hline PDS~2 & 175$^a$ & & & no & 3.98$^{d}$ & 1.68$^{d}$ & 2.5 & \\ HD~47839$^*$& 120$^b$ & & & yes$^{ee}$ & 4.57$^{uu}$ & 5.23$^{uu}$ & & $\sim$0.3$^{eee}$ \\ HD~95881 & 50$^c$ &$-$8.04 & Si, PAH$^r$ & yes$^{ff}$ & 3.86$^{vv}$ & 1.84$^{vv}$ & 3.1 & $>$3$^{x}$ \\ HD~97048 & 140$^d$ &$-$7.17 & PAH$^s$ & no$^{gg}$ & 4.00$^{s}$ & 1.64$^{s}$ & 2.5 & $>$2$^{d}$ \\ HD~97300 & &$<$$-$8.18 & PAH$^t$ & yes$^{hh}$ & 4.02$^{ww}$ & 1.54$^{ww}$ & 2.5 & $>$3$^{ww}$ \\ HD~100453 & 39$^{e}$ &$-$8.04 & PAH$^{u}$ & yes$^{ii}$ & 3.87$^{s}$ & 0.90$^{s}$ & 1.7 & $14\pm4$$^{x}$ \\ HD~100546 & 65$^f$ & & Si, PAH$^{u}$ & no$^{gg}$ & 4.02$^{s}$ & 1.51$^{s}$ & 2.5 & $>$10$^{d}$ \\ HD~101412 & 5$^g$ & & Si, PAH$^{v}$ & yes$^{gg}$ & 3.98$^{xx}$ & 1.74$^{xx}$ & 2.5 & $\sim$2$^{fff}$ \\ HD~135344B & 69$^{h}$ &$-$8.27 & Si$^s$, PAH$^{w}$ & yes$^{jj}$& 3.82$^{s}$ & 0.91$^{s}$ & 1.6& $8\pm 4^{x}$ \\ HD~139614 & 15$^i$ &$-$7.99 & Si$^{u}$ & yes$^{ee}$ & 3.90$^{s}$ & 0.91$^{s}$ & 1.8 & $>$10$^{x}$ \\ HD~144432 & 70$^i$ &$-$7.07 & Si$^{u}$ & yes$^{kk}$ & 3.87$^{s}$ & 1.01$^{s}$ & 1.8 & $10\pm 5^{x}$ \\ HD~144668 & 100$^i$ &$-$6.37 & Si$^{x}$ & yes$^{ll}$ & 3.90$^{s}$ & 1.94$^{s}$ & 3.1 & $0.6\pm 0.4^{ww}$\\ HD~150193 & 100$^f$ &$-$7.29 & Si$^s$ & yes$^{mm}$ & 3.95$^{s}$ & 1.38$^{s}$ & 2.2 & $>$2$^{d}$ \\ HD~152404 & 18.5$^{j}$ & & Si$^{y}$ & yes$^{j}$ & 3.81$^{s}$ & 0.95$^{s}$ & 1.7 & $\sim$8$^{vv}$ \\ HD~158643 & 267$^{h}$/228$^k$ &$-$6.87 & Si$^{u}$ & no$^{nn}$ & 4.00$^{d}$ & 2.39$^{d}$ & 3.9 & 0.3$^{d}$ \\ HD~163296 & 130$^i$ &$-$7.12 & Si$^{u}$ & no$^{gg}$ & 3.94$^{s}$ & 1.38$^{s}$ & 2.2 & $5\pm2$$^{x}$ \\ HD~169142 & 66$^{h}$ &$-$7.40 & PAH$^{w}$ & yes$^{oo}$ & 3.91$^{s}$ & 1.16$^{s}$ & 2.0 & $6\pm3$$^{x}$ \\ VV~Ser & 142$^a$/229$^{l}$ &$-$6.34 & Si$^{z}$ & no$^{gg}$ & 3.95$^{s}$ & 1.27$^{s}$ & 2.0 & $3.5\pm0.5$$^{ggg}$\\ HD~176386 & &$-$8.11 & PAH$^{aa}$ & yes$^{ee}$ & 4.03$^{ww}$ & 1.69$^{ww}$ & 2.7 & $>$2$^{ww}$ \\ HD~179218 & 60$^b$ &$-$6.59 & Si, PAH$^{u}$ & no$^{gg}$ & 4.02$^{s}$ & 2.00$^{s}$ & 3.0 & $1.3\pm0.5$$^{x}$\\ HD~190073 & 12$^i$ & & Si, PAH$^r$ & yes$^{ff}$ & 3.95$^{d}$ & 1.80$^{d}$ & 2.7 & $1.2\pm0.6$$^{hhh}$\\ \hline \multicolumn{9}{c}{Stars with debris disks}\\ HD~9672 & 196$^k$ & & --$^{bb}$ & no & 4.00$^{yy}$ & 1.42$^{yy}$ & 2.3 & $\sim$8$^{iii}$ \\ HD~39060 & 130$^{m}$ & & Si$^{cc}$ & no & 3.91$^{zz}$ & 0.95$^{zz}$ & 1.8 & $\sim$12$^{jjj}$ \\ HD~109573 & 152$^k$ &$<$$-$8.53 & --$^{bb}$ & yes$^{pp}$ & 3.97$^{aaa}$ & 1.32$^{aaa}$ & 2.2 & 8~$\pm$~2$^{pp}$ \\ HD~164249 & & & & yes$^{qq}$ & 3.81$^{bbb}$ & 0.48$^{n}$ & 1.4 & $\sim$12$^{jjj}$ \\ HD~172555 & & & Si$^{dd}$ & no & 3.89$^{bbb}$ & 0.96$^{n}$ & 1.7 & $\sim$12$^{jjj}$ \\ HD~181327 & 16$^{n}$ & & & no & 3.81$^{bbb}$ & 0.54$^{n}$ & 1.4 & $\sim$12$^{jjj}$ \\ \hline \multicolumn{9}{c}{Magnetic Herbig Ae/Be stars from previous studies}\\ HD~31648$^*$ & 90$^{o}$ & & Si$^{s}$ & no$^{rr}$ & 3.94$^{s}$ & 1.14$^{s}$ & 2.0 & $\sim$7$^{kkk}$ \\ HD~104237$^*$ & 10$^{h}$ & $-$7.45 & Si$^{s}$ & yes$^{ss}$ & 3.93$^{s}$ & 1.54$^{s}$ & 2.2 & $2.0\pm0.5$$^{ww}$ \\ HD~200775$^*$ & 26$^{p}$ & & & yes$^{tt}$ & 4.29$^{s}$ & 3.82$^{s}$ & & $0.1\pm0.05$$^{ww}$ \\ V380~Ori & 200$^{f}$ & & Si$^{x}$ & yes$^{ee}$ & 3.97$^{d}$ & 2.04$^{ddd}$ & 3.0 & $1.5\pm0.5$$^{x}$ \\ BF~Ori & 37$^{l}$ & & Si$^{s}$ & no & 3.95$^{s}$ & 1.53$^{s}$ & 2.3 & $\sim$2$^{lll}$ \\ \hline \multicolumn{9}{c}{Standard Ap star with a weak magnetic field}\\ HD~162725 & 32$^q$ & & & & 3.99$^{ccc}$ & 2.33$^{ccc}$ & & \\ \hline \end{tabular}} \par \smallskip 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.~\ref{sect:link}). Objects marked with $^*$ are excluded from the correlation analysis (see Sects.~\ref{sect:observations}, \ref{sect:prev_detect}, and~\ref{subsect:accr_rate}).\\ References: $^a$ Vieira et~al.\ (\cite{Vieira2003}), $^b$ Bernacca \& Perinotto (\cite{BernaccaPerinotto1970}), $^c$ Grady et~al.\ (\cite{Grady1996}), $^d$ van den Ancker et~al.\ (\cite{vandenAncker1998}), $^{e}$ Acke \& Waelkens (\cite{AckeWaelkens2004}), $^f$ Hamidouche et~al.\ (\cite{Hamidouche2008}), $^{g}$ this work, $^{h}$ Dunkin et~al.\ (\cite{Dunkin1997}), $^i$ Hubrig et~al.\ (\cite{Hubrig2007b}), $^{j}$ Alencar et~al.\ (\cite{Alencar2003}), $^k$ Royer et~al.\ (\cite{Royer2007}), $^{l}$ Mora et~al.\ (\cite{Mora2001}), $^{m}$ Slettebak (\cite{Slettebak1982}), $^{n}$ de la Reza \& Pinz\'on (\cite{delaRezaPinzon2004}), $^{o}$ Beskrovnaya et~al.\ (\cite{Beskrovnaya2004}), $^{p}$ Alecian et~al.\ (\cite{Alecian2008}), $^q$ Landstreet et~al.\ (\cite{Landstreet2008}), $^r$ Boersma et~al.\ (\cite{Boersma2008}), $^s$ Acke \& van den Ancker (\cite{Acke2004}), $^t$ Siebenmorgen et~al.\ (\cite{Siebenmorgen1998}), $^{u}$ Meeus et~al.\ (\cite{Meeus2001}), $^{v}$ Geers et~al.\ (\cite{Geers2007}), $^{w}$ Sloan et~al.\ (\cite{Sloan2005}), $^{x}$~van~Boekel et~al.\ (\cite{vanBoekel2005}), $^{y}$ Przygodda et~al.\ (\cite{Przygodda2003}), $^{z}$ Pontoppidan et~al.\ (\cite{Pontoppidan2007b}), $^{aa}$ Siebenmorgen et~al.\ (\cite{Siebenmorgen2000}), $^{bb}$ Kessler-Silacci et~al.\ (\cite{KesslerSilacci2005}), $^{cc}$~Okamoto et~al.\ (\cite{Okamoto2004}), $^{dd}$ Sch\"utz et~al.\ (\cite{Schuetz2005b}), $^{ee}$ Dommanget \& Nys (\cite{Dommanget1994}), $^{ff}$ Baines et~al.\ (\cite{Baines2006}), $^{gg}$ Corporon \& Lagrange (\cite{Corporon1999}), $^{hh}$Stelzer et~al.\ (\cite{Stelzer2006}), $^{ii}$ Chen et~al.\ (\cite{Chen2006a}), $^{jj}$ Augereau et~al.\ (\cite{Augereau2001}), $^{kk}$ Carmona et~al.\ (\cite{Carmona2007}), $^{ll}$ Stecklum et~al.\ (\cite{Stecklum1995}), $^{mm}$ Reipurth \& Zinnecker (\cite{Reipurth1993}), $^{nn}$ Roberge et~al.\ (\cite{Roberge2002}), $^{oo}$ Grady et~al.\ (\cite{Grady2007}), $^{pp}$ Stauffer et~al.\ (\cite{Stauffer1995}), $^{qq}$ SIMBAD, $^{rr}$ Eisner et~al.\ (\cite{Eisner2004}), $^{ss}$ Grady et~al.\ (\cite{Grady2004}), $^{tt}$ Pirzkal et~al.\ (\cite{Pirzkal1997}), $^{uu}$ Schnerr et~al.\ (\cite{Schnerr2007}), $^{vv}$ Blondel et~al.\ (\cite{Blondel2006}), $^{ww}$ van den Ancker et~al.\ (\cite{vandenAncker1997}), $^{xx}$ Wade et~al.\ (\cite{Wade2007}), $^{yy}$ Hughes et~al.\ (\cite{Hughes2008}), $^{zz}$ di Folco et~al.\ (\cite{diFolco2004}), $^{aaa}$ Debes et~al.\ (\cite{Debes2008}), $^{bbb}$ Zuckerman \& Song (\cite{ZuckermanSong2004}), $^{ccc}$ Folsom et~al.\ (\cite{Folsom2007}), $^{ddd}$ Corcoran \& Ray (\cite{CorcoranRay1998}), $^{eee}$ Walsh (\cite{Walsh1980}), $^{fff}$~Wade et~al.\ (\cite{Wade2005}), $^{ggg}$ Pontoppidan et~al.\ (\cite{Pontoppidan2007a}), $^{hhh}$ Catala et~al.\ (\cite{Catala2007}), $^{iii}$ Thi et~al.\ (\cite{Thi2001}), $^{jjj}$ Zuckerman et~al.\ (\cite{Zuckerman2001}), $^{kkk}$ Simon et~al.\ (\cite{Simon2000}), and $^{lll}$ Natta et~al.\ (\cite{Natta1997}). \end{table}