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- W2100635386 abstract "We present NICMOS NIC3 observations of the Galactic globular cluster NGC 288, taken South - East at 2.4 times the cluster's half-light radius in the J and H bands. We have detected the cluster main sequence down to J ' 25 and H ' 24. The corresponding luminosity function covers the range 3 <M H < 9 and peaks at MH ' 6:8. The theoretical tracks of Baraffe et al. (1997) at (F e=H )= 1:3 give a mass function which is best fitted by a log-normal distribution with characteristic mass of mc =0 :42 M and a standard deviation =0 :35. This result is fully consistent with the global mass function derived by Paresce & De Marchi (2000) for a sample of 12 globular clusters with very different dynamical histories, thus confirming that near the cluster's half-light radius the mass function at appears undistorted by evaporation or tidal inter- actions with the Galaxy and should then reflect the initial mass function." @default.
- W2100635386 created "2016-06-24" @default.
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- W2100635386 date "2000-10-01" @default.
- W2100635386 modified "2023-09-25" @default.
- W2100635386 title "The mass function of NGC 288" @default.
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