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- W1561081572 abstract "Translated from Astron. Zh.; 49: No. 6, 1229-1237(1972). Peebles and Dicke's hypothesis for the cosmological origin of globular clusters is applied to consider the possible fragmentation of primordial clouds into stars by thermal instability for a wide range of initial conditions. Thermal instability would cause the central part of a cloud to disintegrate; it would cease to contract because of the passage of weak shock waves heating the material to 2000 to 5000 deg K. If the central cloud temperature is lower, a star with M approximately 10/sup 2/ M/sub sub solar / will be generated. Globular protoclusters will become isolated from the background Friedmann expansion when z > 10, and the most probable epoch for such events would be z approximately 40. (auth)" @default.
- W1561081572 created "2016-06-24" @default.
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- W1561081572 date "1973-01-01" @default.
- W1561081572 modified "2023-10-17" @default.
- W1561081572 title "Cosmological Hypothesis for the Origin of Globular Clusters." @default.
- W1561081572 hasPublicationYear "1973" @default.
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