%Format: latex \documentstyle[referee]{l-aa} \begin{document} \thesaurus{(09.03.1; 09.13.2; 09.01.1)} \title{Further search for OH emission from IRAS sources.} \begin{table}[htb] \caption{Masers. Column 1 contains IRAS names, or other names. Column 2 -- galactic coordinates. Columns 3, 4 and 5 -- Gaussian fits for the 1667~MHz line. Columns 6, 7 and 8 -- Gaussian fits for the 1665~MHz~line. Right and left circular polarizations are designated by R and L, while H and V stand for horizontal and vertical linear polarizations. Capital T is used when a line was supposed to be thermal. } \tiny \begin{center} \vskip 5pt \begin{tabular}{c|c|c|c|c|c|c|c} \hline Source name & \rule{0pt}{10pt}Galactic &\multicolumn{3}{c|}{1667~MHZ} &\multicolumn{3}{c}{1665~MHZ} \\ \cline{3-8} &coordinates & \rule{0pt}{10pt}V, $\rm km~s^{-1}$ & FWHM, $\rm km~s^{-1}$ & Flux, Jy & V, $\rm km~s^{-1}$ & FWHM, $\rm km~s^{-1}$ & Flux, Jy \\ \hline \rule{0pt}{10pt}Cas C1 & 128.5+11.1 & & & & 16.11(0.04) & 0.56(0.41) & 0.44(0.07)L \\ \dots & & 3.22(0.11) & 1.29(0.47) & 0.34(0.06)T & 3.43(0.14) & 1.11(0.25) & 0.27(0.02)T \\ % \dots & & & &&&&&&&\\ Cas D1 & 130.1+11.6 & $-$14.58(0.09) & 1.95(0.22) & 0.36(0.04)T & $-$14.86(0.15) & 1.81(0.34) & 0.24(0.03)T \\ \dots & & & & & 15.19(0.09) & 0.56(0.05) & 0.38(0.06)L \\ \dots & & & & & 15.00(0.05) & 0.56(0.28) & 0.35(0.03)R \\ % \dots & & & &&&&&&&\\ 02460+5929 & 137.4+0.2 & & & $\rm <$0.05 & $-$6.49(0.19) & 1.12(0.26) & 0.16(0.03)L \\ \dots & & & & & $-$6.49(0.20) & 1.13(0.25) & 0.21(0.04)R \\ % \dots & & & &&&&&&&\\ 03414+3200 & 160.5$-$17.8 & 8.79(0.15) & 1.88(0.30) & 0.24(0.04)T & $-$29.26(0.31) & 1.23(0.31) & 0.20(0.03)L \\ \dots & & & & & $-$29.11(0.03) & 1.13(0.06) & 1.6(0.15)R \\ % \dots & & & &&&&&&&\\ 05137+3919 & 168.1+0.8 & & & $\rm <$0.09 & $-$21.42(0.02) & 0.09(0.02) & 0.79(0.15)L \\ \dots & & & & & $-$21.40(0.04) & 0.18(0.01) & 2.65(0.12)R \\ % \dots & & & &&&&&&&\\ 05274+3345 & 174.2$-$0.1 & $-$4.55(0.16) & 1.71(0.26) & 0.23(0.09)L & $-$3.79(0.08) & 1.44(0.31) & 0.34(0.11)L \\ (AFGL5142) & & $-$4.18(0.25) & 3.01(0.56) & 0.13(0.09)R & $-$3.39(0.08) & 1.54(0.11) & 0.68(0.09)R \\ % \dots & & & &&&&&&&\\ 05379+3550$^{\rm a}$ & 173.6+2.9 & $-$21.6 & & $\rm <$0.5 & $-$21.63(0.03) & 0.89(0.07) & 0.61(0.04)L \\ \dots & & & & & $-$26.83(0.01) & 0.59(0.03) & 1.57(0.06)R \\ \dots & & & & & $-$21.71(0.07) & 0.79(0.20) & 0.44(0.06)H \\ \dots & & & & & $-$26.87(0.02) & 0.42(0.05) & 0.69(0.07)V \\ \dots & & & & & $-$26.8 & & $\rm <$0.05L \\ \dots & & & & & $-$21.7 & & $\rm <$0.05R \\ % \dots & & & &&&&&&&\\ 05480+2545 & 183.3$-$0.6 & $-$3.89(0.03) & 0.56(0.20) & 0.43(0.03)L & $-$12.88(0.03) & 0.57(0.45) & 0.52(0.04)L \\ \dots & & $-$4.52(0.24) & 0.56(0.30) & 0.28(0.02)R & $-$15.28(0.07) & 0.56(0.52) & 0.19(0.05)R \\ \dots & & $-$9.16(0.27) & 2.20(0.60) & 0.13(0.03)R & $-$5.94(0.30) & 0.54(0.30) & 0.40(0.15)R \\ \dots & & $-$18.87(0.31) & 2.08(1.34) & 0.09(0.03)R & $-$4.81(0.29) & 0.47(0.22) & 0.75(0.30)R \\ % \dots & & & &&&&&&&\\ 06446+0029 & 212.1$-$0.7 & & & $\rm <$0.2 & 48.65(0.01) & 0.25(0.01) & 4.76(0.28)L \\ \dots & & & & & 48.96(0.07) & 0.43(0.11) & 0.83(0.09)L \\ \dots & & & & & 48.64(0.01) & 0.26(0.01) & 4.90(0.22)R \\ \dots & & & & & 48.96(0.05) & 0.36(0.09) & 1.00(0.11)R \\ % \dots & & & &&&&&&&\\ 07111$-$1211 & 226.4$-$0.8 & 16.54(0.24) & 2.93(0.56) & 0.12(0.02)L & 16.40(0.19) & 2.19(0.45) & 0.12(0.02)L \\ \dots & & 16.72(0.21) & 2.76(0.51) & 0.16(0.03)R & 16.22(0.07) & 1.12(0.20) & 0.26(0.05)R \\ % \dots & & & &&&&&&&\\ 07427$-$2400 & 240.3+0.1 & 63.93(0.02) & 0.33(0.05) & 0.57(0.07)L & 62.94(0.01) & 0.23(0.02) & 1.62(0.15)L \\ \dots & & 63.96(0.01) & 0.06(0.02) & 0.41(0.12)R & 63.31(0.02) & 0.43(0.11) & 1.20(0.05)L \\ \dots & & & & & 63.65(0.01) & 0.22(0.01) & 1.97(0.19)L \\ \dots & & & & & 63.05(0.02) & 0.29(0.03) & 5.04(0.22)R \\ \dots & & & & & 63.32(0.01) & 0.20(0.04) & 3.81(0.52)R \\ \dots & & & & & 63.60(0.04) & 0.31(0.09) & 1.58(0.21)R \\ \dots & & & & & & & \\ \dots & & & & $\rm <$0.7H & 63.05(0.03) & 0.35(0.06) & 1.92(0.13)V \\ \dots & & & & & 63.33(0.02) & 0.19(0.05) & 1.49(0.30)V \\ \dots & & & & & 63.62(0.02) & 0.21(0.04) & 1.36(0.17)V \\ \dots & & 63.91(0.03) & 0.31(0.08) & 0.44(0.09)V & 63.02(0.02) & 0.30(0.04) & 2.56(0.23)H \\ \dots & & & & & 63.31(0.02) & 0.23(0.06) & 2.90(0.36)H \\ \dots & & & & & 63.61(0.03) & 0.27(0.06) & 2.26(0.22)H \\ % \dots & & & &&&&&&&\\ 07528$-$3441$^{\rm b}$ & 250.6$-$3.5 & & & $\rm <$0.02 & $-$26.30(0.01) & 0.14(0.09) & 0.44(0.05)L \\ \dots & & & & & $-$26.30(0.02) & 0.14(0.22) & 0.30(0.07)R \\ % \dots & & & &&&&&&&\\ 17269$-$2235 & 3.5+6.3 & 62.50(0.08) & 3.11(0.45) & 0.60(0.09) & 63.50(0.07) & 1.50(0.31) & 0.9(0.07)$\rm ^{\rm c}$ \\ \dots & & 99.50(0.11) & 2.09(0.23) & 2.11(0.10) & 98.50(0.13) & 1.6(0.17) & 0.75(0.09)$\rm ^{\rm c}$ \\ % \dots & & & &&&&&&&\\ 17416$-$2112 & 6.5+4.2 & 25.06(0.08) & 1.12(0.59) & 0.20(0.13) & 38.23(0.74) & 12.77(1.54) & 0.05(0.01) \\ \dots & & 55.76(0.02) & 1.26(0.05) & 0.69(0.13) & & & \\ % \dots & & & &&&&&&&\\ 17576$-$1845 & 10.5+2.2 & 23.58(0.05) & 0.83(0.19) & $-$0.26(0.03) & 18.98(0.05) & 0.56(0.07) & 0.38(0.03)L \\ &&&&&&&\\ 17579$-$3121 & 359.6$-$4.1 & $-$10.83(0.14) & 2.98(0.36) & 0.24(0.03) & & & $\rm <$0.07 \\ \dots & & 32.90(0.30) & 3.92(0.69) & 0.13(0.03) & & & \\ % \dots & & & &&&&&&&\\ 17589$-$2312 & 6.8$-$0.3 & 16.74(0.11) & 1.60(0.32) & 1.27(0.12)L & 13.69 & 0.9 & 2.13L \\ \dots & & 15.57(0.09) & 1.26(0.43) & 0.85(0.13)R & 15.37 & 1.07 & 4.60L \\ \dots & & & & & 16.49 & 1.07 & 4.74L \\ \dots & & & & & 16.49 & 0.9 & 0.74R \\ \dots & & & & & 21.43 & 0.79 & 0.57R \\ % \dots & & & &&&&&&&\\ 20049+2725 & 68.8$-$2.5 & 6.12(0.45) & 3.83(1.09) & 0.1(0.02)L & 6.28(0.25) & 3.27(0.39) & 0.19(0.02)L \\ \dots & & 14.54(0.33) & 1.13(0.42) & 0.12(0.03)L & 6.14(0.16) & 3.35(0.41) & 0.24(0.03)R \\ \dots & & 6.58(0.60) & 4.36(1.24) & 0.07(0.02)R & & & \\ \dots & & 14.23(0.12) & 1.13(0.20) & 0.10(0.02)R & & & \\ % \dots & & & &&&&&&&\\ 20144+3526 & 73.7+0.8 & $-$71.14(0.10) & 0.63(0.16) & 0.15(0.07)L & $-$75.62(0.03) & 0.64(0.04) & 0.58(0.15)L \\ \dots & & $-$75.14(0.16) & 0.56(0.45) & 0.11(0.02)R & $-$72.36(0.04) & 0.63(0.08) & 0.55(0.12)L \\ \dots & & $-$70.05(0.07) & 0.56(0.24) & 0.14(0.02)R & $-$66.93(0.11) & 0.81(0.18) & 0.20(0.16)L \\ \dots & & & & & $-$75.60(0.03) & 0.65(0.05) & 0.65(0.21)R \\ \dots & & & & & $-$68.81(0.12) & 0.92(0.31) & 0.20(0.21)R \\ % \dots & & & &&&&&&&\\ 20361+5733 & 93.9+10.0 & $-$1.60(0.13) & 1.28(0.28) & 0.13(0.04)L & $-$1.54(0.13) & 1.64(0.38) & 0.17(0.01)L \\ \dots & & 14.95(0.26) & 1.16(0.58) & 0.07(0.04)L & $-$1.30(0.13) & 1.84(0.26) & 0.22(0.01)R \\ \dots & & $-$1.64(0.19) & 1.38(0.41) & 0.14(0.05)R & & & \\ \dots & & 15.07(0.23) & 1.23(0.28) & 0.12(0.05)R & & & \\ % \dots & & & &&&&&&&\\ 20436+5849 & 95.5+9.9 & $-$2.29(0.04) & 0.79(0.06) & 0.39(0.03) & $-$2.36(0.08) & 0.88(0.12) & 0.24(0.04) \\ \dots & & 3.31(0.10) & 0.85(0.17) & 0.13(0.01) & & & $\rm < 0.04$ \\ % \dots & & & &&&&&&&\\ 21246+5512 & 96.6+3.4 & & & $\rm <$0.05 & 10.49(0.24) & 1.20(0.43) & 0.11(0.04)L \\ \dots & & & & & 10.35(0.26) & 1.13(0.78) & 0.12(0.03)R \\ % \dots & & & &&&&&&&\\ 21432+4719 & 93.5$-$4.4 & 4.01(0.13) & 1.61(0.33) & 0.13(0.04) & 3.69(0.31) & 1.47(0.44) & 0.08(0.03) \\ \dots & & 21.02(0.36) & 1.40(0.23) & 0.05(0.02) & 19.22(0.23) & 1.12(0.09) & 0.09(0.02) \\ % \dots & & & &&&&&&&\\ 22051+5848 & 103.1+2.7 & & & $\rm <$0.03 & 8.46(0.07) & 1.13(0.40) & 0.13(0.01)L \\ \dots & & & & & 8.50(0.09) & 1.13(0.13) & 0.08(0.02)R \\ % \dots & & $-$1.71(0.15) & %1.30(0.44) & 0.08(0.01)T & & % & & & \\ \dots & & $-$1.71(0.15) & 1.30(0.44) & 0.08(0.01)T &&&\\ \hline \end{tabular} \end{center} \rule{2cm}{0cm}$\footnotesize\rm ^a$\rule{0pt}{11pt}\footnotesize 1665~V~profile centered at -21~$\rm km~s^{-1}$ and 1665~H~profile at -27~$\rm km~s^{-1}$\\ \rule{2cm}{0cm} were not observed with high velocity resolution.\\ \rule{2cm}{0cm}$\rm ^b$\rule{0pt}{11pt}\footnotesize Detection reported in the Paper I.\\ \rule{2cm}{0cm}$\rm ^c$\rule{0pt}{11pt}\footnotesize These are parameters of 1612~MHz OH line. \end{table} \begin{table}[htb] \rm \caption{Thermal sources. Column 1 contains IRAS or other names. Column 2 -- associations of an IRAS source with nebulae of Lynds. Column 3 -- galactic coordinates. Columns 4, 5, 6 and 7 -- results of Gaussian fits. Column 8 contains estimates of OH column density. Column 10 and 11 -- CO radial velocities with the corresponding references. Column 11 -- name of a associated IRAS cloud or core (Wood~et~al.~1994)} \begin{center} \vskip 10pt \begin{tabular}{l|c|c|c|c|c|c|c|c|c|c} \hline \multicolumn{3}{c|}{Source Name}&\multicolumn{2}{c|}{Flux, Jy}& \rule{0pt}{11pt}V & FWHM&N$\rm _{OH},$&V(CO) &CO&IRAS cloud\\ \cline{1-5} \rule{0pt}{11pt}IRAS & Lynds & Galactic& 1667 & 1665 & $\rm km\,s^{-1}$ & $\rm km\,s^{-1}$ &10$\rm ^{14}$cm$^{-2}$& $\rm km\,s^{-1}$ & Ref. & or core\\ \hline \rule{0pt}{11pt}03220+3035& 1448 & 157.9$-$21.5 & 0.15 & 0.07 & 4.1 & 1.2 & 2.84 & & & Per A \\ PerA11 & \dots & 157.8$-$20.7 & 0.06 & 0.09 & 0.9 & 3.8 & 1.18 & & &PerA11 \\ & & & 0.10 & 0.08 & 7.8 & 1.2 & 0.62 & & & \\ 03245+3002 & 1455 & 158.8$-$21.6 & 0.30 & 0.13 & 7.9 & 2.1 & 8.97 & & & \\ 03262+3108 & 1450 & 158.4$-$20.5 & 0.25 & 0.09 & 7.8 & 2.4 & 9.59 & 8.4 & [1] & Per A2 \\ 03439+3233 & 1471 & 160.7$-$17.2 & 0.12 & $\rm<$0.06 & 9.9 & 1.0 & 2.71 & & & Per A \\ 04016+2610 & 1491 & 168.1$-$19.2 & 0.13 & 0.07 & 7.0 & 1.3 & 2.14 & 7 & [2] & Tau K1 \\ 04073+3800 & 1473 & 160.5$-$9.8 & 0.26 & 0.11 & $-$3.3 & 1.4 & 4.54 & & & \\ 04191+1523 & \dots & 179.6$-$23.5 & 0.15 & 0.11 & 6.8 & 0.9 & 2.94 & & & \\ 04263+2426 & 1529 & 173.4$-$16.3 & 0.35 & 0.19 & 6.4 & 1.8 & 9.61 & 6.5 & [2] & Tau E1 \\ 04269+3507 & 1482 & 165.4$-$0.9 & 0.12 & $\rm<$0.06 & $-$0.2 & 2.1 & 3.18 & $-$1 & [3] & \\ 04278+2435 & 1529 & 173.5$-$16.0 & 0.19 & 0.08 & 6.2 & 1.4 & 4.54 & 6.2 & [4] & \\ 04287+1807 & 1551 & 178.7$-$20.1 & 0.17 & 0.08 & 6.8 & 1.7 & 3.06 & 6.84 & [1] & \\ 04325$-$1419 & 1642 & 210.8$-$36.6 & 0.19 & 0.07 & 0.4 & 1.3 & 3.06 & & & \\ 04325+2402 & 1535 & 174.7$-$15.5 & 0.27 & 0.10 & 5.7 & 1.2 & 4.55 & 5.7 & [2] & Tau 51 \\ 04360+2610 & 1527 & 173.5$-$13.5 & 0.32 & 0.27 & 6.1 & 1.1 & 5.34 & & & \\ 04369+2539 & 1534 & 174.1$-$13.7 & 0.38 & 0.29 & 6.2 & 1.2 & 8.89 & 6.82 & [1] & Tau A1 \\ 05075+3755 & \dots & 168.6$-$1.0 & 0.09 & 0.05 & $-$16.6 & 1.5 & 1.85 & & [5] & \\ 05168+3634 & \dots & 170.7$-$0.3 & 0.06 & 0.07 & $-$16.2 & 4.1 & 2.77 & $-$15 & [5] & \\ 05271+3509 & \dots & 176.5$-$1.7 & 0.16 & 0.13 & $-$19.5 & 2.3 & 4.65 & $-$19.6 & [5] & \\ 05283$-$0412 & 1640 & 207.3$-$19.8 & 0.22 & 0.13 & 11.0 & 2.3 & 4.16 & 10 & & \\ RNO 43 & \dots & 192.1$-$11.0 & 0.14 & & 10.1 & 0.7 & 2.03 & & & \\ 05387$-$0924 & 1647 & 213.5$-$19.9 & $\rm<$0.12 & 0.18 & 3.9 & 2.2 & 9.28 & & & \\ 05389$-$0756 & 1641 & 212.1$-$19.2 & 0.76 & 0.56 & 5.0 & 2.2 & 30.37 & & & \\ 05435$-$0015 & 1627 & 205.1$-$14.4 & 0.21 & 0.10 & 10.0 & 1.6 & 4.68 & & & Ori A1 \\ 05487+0255 & 1617 & 203.3$-$11.9 & 0.06 & 0.05 & 8.5 & 1.1 & 0.82 & & & Ori A34 \\ 05491+0247 & 1617 & 203.5$-$11.9 & 0.09 & 0.05 & 9.0 & 2.3 & 2.56 & & & Ori A2 \\ 05496+0812 & 1598 & 198.7$-$9.2 & 0.08 & 0.05 & 11.2 & 2.2 & 2.33 & 13.33 & [5] & Ori J \\ 06046$-$0603 & 1646 & 213.3$-$12.6 & 0.10 & 0.05 & 11.9 & 3.3 & 5.03 & & & \\ 06067+2138 & \dots & 189.0+1.0 & 0.16 & 0.11 & 2.3 & 4.0 & 22.17 & 3.2 & [5] & \\ 06306+0437 & \dots & 206.8$-$1.9 & $-$0.10 & $-$0.09 & 14.3 & 5.5 & & 13.97 & [5] & \\ 06308+0402 & \dots & 207.3$-$2.2 & $-$0.04 & $-$0.05 & 0.8 & 5.5 & & 7.56 & [5] & \\ 06343$-$1036 & \dots & 220.8$-$8.1 & 0.06 & 0.04 & 12.7 & 4.2 & 4.46 & & & Mon A \\ 06587$-$0859 & 1654 & 222.1-2.0 & 0.12 & $\rm<$0.05 & 40.2 & 2.4 & 3.21 & & & \\ 07020$-$1618 & \dots & 229.0$-$4.6 & 0.07 & 0.04 & 19.5 & 1.6 & 1.17 & 19.58 & [5] & \\ 07077$-$1026 & \dots & 224.4$-$0.7 & 0.22 & 0.08 & 15.5 & 2.0 & 5.68 & 14.1 & [5] & \\ 07173$-$1744 & \dots & 231.9$-$2.1 & 0.07 & $\rm<$0.06 & 43.4 & 2.9 & 2.36 & 41.3 & [5] & \\ & & & 0.06 & $\rm<$0.03 & 48.0 & 1.2 & 0.83 & & & \\ %\hline %\end{tabular} %\end{center} %\end{table} %\newpage %\addtocounter{table}{-1} %\begin{table}[htb] %\caption{\it {} continued} %\begin{center} %\vskip 10pt %\begin{tabular}{l|c|c|c|c|c|c|c|c|c|c} %\hline %\multicolumn{3}{c|}{Source Name}&\multicolumn{2}{c|}{Flux}& V & %FWHM&N$_{OH},$&V(CO)&CO&IRAS cloud\\ %\cline{1-5} %IRAS & Lynds & Galactic& 1667 & 1665 & & &10$^{14}$cm$^{-2}$& & Ref. & or core\\ %\hline 07422$-$2001 & \dots & 236.8+2.0 & 0.08 & 0.08 & 52.3 & 3.3 & 1.62 & 52.7 & [5] & \\ 16235$-$2416 & 1688 & 353.1+16.9 & 0.30 & $\rm<$0.05 & 3.9 & 2.3 & 9.45 & 3.03 & [6] & Oph A1 \\ 16242$-$2422 & 1688 & 353.1+16.7 & 0.64 & 0.56 & 3.7 & 1.6 & 22.02 & 3.03 & & Oph A2 \\ 16244$-$2432 & 1688 & 353.0+16.6 & 0.55 & 0.38 & 3.6 & 1.5 & 14.53 & 3.5 & [2] & Oph A3 \\ 16288$-$2450 & \dots & 353.5+15.6 & 0.25 & 0.12 & 4.2 & 1.1 & 3.84 & 4.35 & [7] & Oph A4 \\ 16341$-$1022 & \dots & 6.3+23.1 & 0.07 & $\rm<$0.04 & $-$1.1 & 0.6 & & & & \\ 16442$-$0930 & 260;261 & 8.7+22.2 & 0.12 & 0.08 & 3.7 & 1.2 & 1.61 & 3.4 & [1] & \\ CTB 37 B & \dots & 348.8+0.2 & $-$0.15 & $-$0.12 & $-$7.6 & 3.2 & & & & \\ & & & 0.12 & $\rm<$0.06 & 0.8 & 3.4 & 5.48 & & & \\ 17130$-$2053 & 100 & 3.1+9.9 & 0.11 & 0.07 & 1.8 & 1.1 & 1.70 & & & \\ 18265+0028 & 570 & 30.8+5.2 & 0.22 & 0.12 & 8.3 & 1.8 & 3.12 & & & \\ 19005$-$0445 & \dots & 30.1$-$4.7 & 0.08 & $\rm<$0.05 & 36.9 & 4.9 & 4.62 & & & \\ 20094+2744 & 824 & 66.6$-$3.2 & 0.14 & 0.1 & 5.3 & 2.9 & 5.55 & & & \\ 20231+3440 & 870 & 74.0$-$1.7 & 0.15 & 0.12 & 5.8 & 3.1 & 6.55 & & & \\ 20568+5217 & 1003 & 91.6+4.4 & 0.22 & 0.11 & $-$3.5 & 3.3 & 10.26 & $-$3 & [3] & \\ 21007+4951 & \dots & 90.2+2.3 & 0.14 & 0.12 & $-$0.8 & 4.5 & 6.27 & 1.1 & [5] & \\ 21025+5221 & 1011 & 92.3+3.8 & 0.23 & 0.16 & $-$1.7 & 3.0 & 9.07 & & & \\ 21106+5206 & 1022 & 92.9+2.7 & $-$0.48 & $\rm<$0.07 & $-$2.3 & 2.1 & & & & \\ & & & $-$0.2 & $-$0.17 & $-$12.1 & 2.6 & & & & \\ 21161+6141 & 1125 & 100.4+8.8 & 0.12 & 0.1 & 0.9 & 3.5 & 5.20 & & & \\ 21429+4726 & 1040 & 93.5$-$4.3 & 0.09 & 0.07 & 3.9 & 0.8 & 1.48 & 4 & [5] & \\ \hline \multicolumn{11}{l}{\rule{0pt}{11pt} \footnotesize [1] Myers et al.(1983), [2] Terebey et al.(1989), [3] Casoli et al.(1986), [4] Heyer et al.(1987), }\\ \multicolumn{11}{l}{\rule{0pt}{11pt} \footnotesize [5] Wouterloot and Brand (1989), [6] de Geus et al.(1990), [7] Benson et al.(1989) }\\ \end{tabular} \end{center} \end{table} \end{document}