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- W1616640854 abstract "Star clusters are extremely common in the Magellanic Clouds. About 120 are known in the SMC, and more than 1600 in the LMC. The true number there has been estimated by Hodge and Sexton (1966) to be about 6000, this total referring to clusters with brightest stars brighter than M B=2. The outermost recognised members of the Cloud system are clusters, Lindsay 1 on the western side being 30°, or at least 30 kpc, from NGC 2257 on the eastern side. Attempts have been made to fit the Cloud clusters into some sort of structural pattern, without success; so far, no analogue has emerged in the Clouds to the galactic system of a narrow disk containing the young clusters surrounded by a spheroidal distribution of old clusters." @default.
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- W1616640854 date "1971-01-01" @default.
- W1616640854 modified "2023-09-27" @default.
- W1616640854 title "Clusters in the Magellanic Clouds" @default.
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- W1616640854 doi "https://doi.org/10.1007/978-94-015-6906-4_4" @default.
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