Zusammenfassung
This paper is concerned
-
(1)
with the processes of formation of stars out of the interstellar gas and dust,
-
(2)
with the properties of clusters and associations of stars,
-
(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)
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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