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- W3046758468 abstract "Plates taken with the 1.2m U.K. Schmidt Telescope and the 3.8 AAT Telescope have been used in order to derive the dynamical parameteres of 43 various clusters of the SMC by means of star counts. The clusters are divided into two main categories: (i) the disk, “blue” and “intermediate” in colour, young, mainly globulars and (ii) the halo, “red”, old globular clusters. The disk clusters have been found to be more massive and older than the galactic open clusters, whereas the halo clusters are at least 10 times less massive than the galactic globulars. The relaxation times of the disk clusters are larger than their evolutionary age while the observed density profiles always show evidence of well relaxed systems." @default.
- W3046758468 created "2020-08-07" @default.
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- W3046758468 date "1984-01-01" @default.
- W3046758468 modified "2023-09-25" @default.
- W3046758468 title "Masses and Relaxation Times of Star Clusters in the SMC" @default.
- W3046758468 cites W2016888075 @default.
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- W3046758468 doi "https://doi.org/10.1017/s0074180900039772" @default.
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