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Zusammenfassung

This paper is concerned

  1. (1)

    with the processes of formation of stars out of the interstellar gas and dust,

  2. (2)

    with the properties of clusters and associations of stars,

  3. (3)

    with the evolution which can take place in these clusters and the theoretical attempts which have been made to explain this evolution, and

  4. (4)

    with the spatial and velocity distributions of different types of stars, as indicators of the ages and past histories of stars.

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Burbidge, G.R. (1960). The Formation of Stars by the Condensation of diffuse Matter. In: Die Entstehung von Sternen durch Kondensation Diffuser Materie. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-662-01328-1_1

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