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- W2316988544 abstract "The dynamical evolution of young star clusters and associations is an evolving interplay of the gravitational potential, as determined by the spatial distribution of volume densities and the motions of both the gas and stars. In this chapter we briefly discuss several nearby star-forming regions which are relevant to our discussion on the dynamics of these young systems, concentrating on those which have been intensively investigated, namely the Taurus-Auriga star-forming region, the Orion Molecular Cloud and the statistical properties of young embedded clusters." @default.
- W2316988544 created "2016-06-24" @default.
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- W2316988544 date "2015-01-01" @default.
- W2316988544 modified "2023-09-26" @default.
- W2316988544 title "Overview of Star-Forming Regions" @default.
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- W2316988544 doi "https://doi.org/10.1007/978-3-662-47290-3_12" @default.
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