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- W63630892 abstract "In spite of all the attempts to find them, no one has yet detected any brown dwarf in a globular cluster. Although powerful instruments such as the VLT and Advanced Camera could further push the frontiers of this search, globular clusters will probably hold tight to their secrets for a while longer. Nonetheless, the search for very low mass stars in globular clusters has taught us a lot about their original mass distribution (IMF) and its evolution in time. I shall review the results of an investigation carried out over what is presently the largest, most homogeneous sample, and discuss the reasons suggesting that: 1. dynamical evolution (internal and external) has reshaped the cluster mass function over time, but the imprint of the IMF is still visible; 2. the IMF appears to vary very little from cluster to cluster; 3. the most likely functional form of the IMF is that of a power law that rises to a peak at ˜ 0.3 M ⊙ and tapers off at smaller masses." @default.
- W63630892 created "2016-06-24" @default.
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- W63630892 date "2003-01-01" @default.
- W63630892 modified "2023-09-25" @default.
- W63630892 title "Globular Clusters: Low Mass Stars, Still No Brown Dwarfs!" @default.
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- W63630892 doi "https://doi.org/10.1017/s0074180900210620" @default.
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