Abstract
Supernova-driven galactic wind and metal enrichment in spheroidal star systems are considered within the general framework of the closed one-zone-model approach. Three issues are addressed: i) protogalaxy binding energy, ii) non-uniform gas density distribution, iii) presence of dark matter. Models of a galaxy with a mass of 1010 M ⊙ are discussed for illustrative purposes.
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© 1990 Kluwer Academic Publishers
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Angeletti, L., Giannone, P. (1990). The Early Evolution of Spheroidal Star Systems. In: Capuzzo-Dolcetta, R., Chiosi, C., di Fazio, A. (eds) Physical Processes in Fragmentation and Star Formation. Astrophysics and Space Science Library, vol 162. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0605-1_23
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DOI: https://doi.org/10.1007/978-94-009-0605-1_23
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