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Table 7:

Stellar mass estimate for clusters older than 50 Myr.
    Observed in CMD   Extrapolated
Cluster   $\Delta~m_{\rm MS}$ $\chi$ $N_{\rm MS}$ $M_{\rm MS}$ $N_{\rm evol}$ $M_{\rm evol}$   N M
    ($M_\odot$)   (stars) ($M_\odot$) (stars) ($M_\odot$)   (stars) ($M_\odot$)
(1)   (2) (3) (4) (5) (6) (7)   (8) (9)
FSR 735   0.55-2.90 $1.21\pm0.11$ $111\pm14$ $164\pm20$ $5\pm1$ $15\pm3$   $1200\pm889$ $467\pm166$
FSR 852   0.65-2.10 $2.59\pm0.46$ $132\pm19$ $152\pm22$ $4\pm6$ $8\pm12$   $2710\pm2190$ $836\pm409$
FSR 953   0.85-2.50 $2.41\pm0.29$ $108\pm14$ $178\pm21$ $8\pm3$ $16\pm6$   $5020\pm3850$ $1670\pm719$
Cz 22     1.30-3.90 $0.87\pm0.20$ $60\pm10$ $135\pm21$ $5\pm3$ $15\pm11$   $1790\pm1290$ $777\pm239$
FSR 941   1.70-2.90 $0.67\pm0.12$ $147\pm13$ $350\pm31$ $40\pm15$ $106\pm39$   $13800\pm10200$ $5480\pm1910$
NGC 2234   0.95-6.75 $0.97\pm0.10$ $139\pm8$ $431\pm28$ $4\pm2$ $32\pm18$   $2640\pm1860$ $1360\pm344$

Notes.  Column 2: MS mass range. Column 3: MS mass function slope $\chi$, derived from the fit of $\phi(m)\propto{m}^{-(1+\chi)}$. Columns 4-7: stellar content of the MS and evolved stars. Columns 8-9: stellar content extrapolated to $0.08~M_{\odot}$.


Source LaTeX | All tables | In the text

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