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Table 3:

Stellar mass estimate.
    Observed in CMD   Extrapolated
Cluster   $\Delta~m_{\rm MS}$ $\chi$ $N_{\rm MS}$ $M_{\rm MS}$ $N_{\rm evol}$ $M_{\rm evol}$   $M_{\rm clus}$ $\rho$
    ($M_\odot$)   (stars) ($M_\odot$) (stars) ($M_\odot$)   ( $10^2~M_\odot$) $(\mbox{$M_\odot$ }~\rm pc^{-3})$
(1)   (2) (3) (4) (5) (6) (7)   (8) (9)
Quality 1
Teu 7   2.5-3.5 $0.85\pm0.63$ $85\pm9$ $262\pm28$ $65\pm15$ $209\pm48$   $21\pm10$ $0.90\pm0.44$
Teu 11   1.7-2.7 $\dagger$ $19\pm4$ $40\pm8$ $5\pm3$ $13\pm9$   $3.3\pm1.3$ $3.22\pm1.26$
Teu 12   1.9-3.5 $\dagger$ $28\pm5$ $83\pm16$ $7\pm3$ $21\pm9$   $4.9\pm1.9$ $0.19\pm0.07$
Teu 13   1.1-9.3 $0.44\pm0.25$ $23\pm4$ $88\pm17$ - -   $1.0\pm0.4$ $1.71\pm0.62$
Teu 14a   0.8-5.3 $0.32\pm0.20$ $70\pm6$ $234\pm21$ $3\pm2$ $14\pm10$   $2.1\pm0.4$ $10.3\pm2.2$
Teu 27   1.1-2.5 $1.63\pm0.72$ $33\pm6$ $57\pm9$ $3\pm1$ $7\pm2$   $2.4\pm1.0$ $25.5\pm10.9$
Teu 40   1.1-2.3 $1.40\pm0.91$ $76\pm7$ $126\pm12$ $17\pm6$ $38\pm14$   $5.5\pm2.3$ $12.4\pm5.2$
Teu 48   1.7-2.9 $\dagger$ $23\pm5$ $58\pm13$ $12\pm8$ $32\pm21$   $3.8\pm1.4$ $0.50\pm0.18$
Teu 49   0.9-2.3 $1.32\pm0.20$ $132\pm9$ $246\pm18$ $19\pm7$ $42\pm16$   $6.4\pm2.3$ $1.46\pm0.52$
Teu 52   0.9-2.7 $0.87\pm0.14$ $36\pm5$ $70\pm10$ $5\pm2$ $15\pm6$   $1.4\pm0.4$ $3.11\pm0.83$
Teu 54   1.1-2.3 $1.04\pm0.18$ $111\pm9$ $180\pm14$ $7\pm5$ $15\pm11$   $6.3\pm2.1$ $3.83\pm1.26$
Teu 64   0.8-2.3 $1.35\pm0.33$ $41\pm5$ $66\pm8$ $2\pm1$ $4\pm2$   $1.5\pm0.6$ $4.60\pm1.75$
Teu 66   2.9-4.1 $1.25\pm0.32$ $44\pm6$ $146\pm20$ $3\pm2$ $12\pm4$   $19\pm8$ $18.5\pm7.8$
Teu 79   1.7-2.9 $0.92\pm0.46$ $75\pm8$ $156\pm17$ $13\pm6$ $32\pm14$   $8.3\pm3.1$ $388\pm143$
Teu 126   0.6-2.9 $1.65\pm0.11$ $89\pm11$ $121\pm14$ $5\pm3$ $15\pm8$   $2.2\pm0.9$ $4.25\pm1.84$
Teu 144   0.9-2.3 $0.61\pm0.22$ $184\pm11$ $278\pm17$ $30\pm7$ $66\pm16$   $5.6\pm1.3$ $6.06\pm1.47$
Quality 2
Teu 2   0.9-1.9 $1.67\pm0.20$ $62\pm6$ $87\pm9$ $3\pm1$ $7\pm2$   $2.6\pm1.1$ $2.56\pm1.05$
Teu 28   1.1-2.3 $1.66\pm0.50$ $47\pm6$ $83\pm11$ $6\pm3$ $13\pm7$   $3.4\pm1.4$ $10.5\pm4.2$
Teu 31   1.5-2.7 $\dagger$ $22\pm3$ $44\pm7$ $3\pm2$ $7\pm6$   $2.7\pm1.0$ $126\pm48$
Teu 43   1.3-1.7 $\dagger$ $12\pm3$ $18\pm4$ $4\pm2$ $7\pm4$   $1.6\pm0.6$ $173\pm29$
Teu 44   1.7-2.5 $\dagger$ $28\pm15$ $63\pm10$ $19\pm7$ $43\pm18$   $5.7\pm2.7$ $1.71\pm0.79$
Teu 50   0.9-1.5 $\dagger$ $25\pm5$ $32\pm6$ $5\pm2$ $7\pm3$   $1.3\pm0.5$ $3.27\pm1.28$
Teu 77   0.9-1.5 $1.48\pm0.93$ $66\pm12$ $69\pm13$ $3\pm1$ $5\pm1$   $3.9\pm1.8$ $28\pm13$
Teu 85   1.3-2.5 $\dagger$ $48\pm5$ $93\pm9$ $23\pm5$ $56\pm13$   $4.9\pm1.7$ $342\pm117$
Teu 106   2.1-2.7 $\dagger$ $14\pm4$ $33\pm9$ $50\pm10$ $124\pm24$   $6.2\pm2.2$ $5.05\pm1.78$
Teu 124   0.9-1.1 $\dagger$ $19\pm3$ $20\pm3$ $14\pm5$ $15\pm5$   $1.9\pm0.8$ $356\pm156$

Notes.  Column 2: detected MS mass range. Column 3: MS mass function slope $\chi$, from $\phi(m)\propto{m}^{-(1+\chi)}$; ($\dagger$): MF slope taken from Kroupa's (2001) IMF. Columns 4-7: MS and evolved stars stellar content. Columns 8-9: cluster mass and density, after MF extrapolation to $0.08~M_{\odot}$.


Source LaTeX | All tables | In the text

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